Updated on 2024/04/11

写真a

 
KANDA Nobuyuki
 
Organization
Graduate School of Science Department of Physics Professor
School of Science Department of Physics
Title
Professor
Affiliation
Institute of Science

Position

  • Graduate School of Science Department of Physics 

    Professor  2022.04 - Now

  • School of Science Department of Physics 

    Professor  2022.04 - Now

Degree

  • Ph.D ( Osaka University )

Research Areas

  • Natural Science / Theoretical studies related to particle-, nuclear-, cosmic ray and astro-physics  / Gravitational Wave Experiment

  • Natural Science / Experimental studies related to particle-, nuclear-, cosmic ray and astro-physics  / 重力波観測

  • Natural Science / Astronomy  / 重力波天文学、重力波天体物理学

Research Interests

  • Gravitational Wave Observation

  • Astrophysics

  • Gravitational Wave Observation

  • Data Analysis of Gravitational Waves

  • Astrophysics

Research subject summary

  • 宇宙にはさまざまな天体がありますが、なかには超新星爆発や中性子星やブラックホール連星の合体といった、天体が劇的な終焉を迎える現象があります。こうした現象では、星の周りの時間と空間が歪み、さざなみのように宇宙に伝わってゆきます。すなわち、アインシュタインの一般相対性理論で予言された“重力波"です。 私たちはレーザーをつかった干渉計という装置を用います。測っている時空の歪みは、原子核よりも小さな距離の変化になります。現在の干渉計は私たちの地球をふくむ銀河系やちかくの銀河でおこった重力波をとらえることができるようになりました。 重力波の形や大きさを測ることによって、たとえば中性子星の重さ(質量)や星までの距離、あるいは星の固さといった、いままでの天文観測とは違った新しい情報が得られると期待されています。

Research Career

  • Gravitational Wave Astrophysics/Astronomy

    Gravitational Wave Astrophysics, Gravitational Wave Astronomy  International Joint Research

    2002.04 - Now 

  • Gravitational Wave Observation

    Gravitational Wave Observation  International Joint Research

    1993.04 - Now 

  • Event Search and Coincidence Analysis of Laser Interferometr

    Gravitational Waves, Laser Interferometer, Black-hole  Joint Research in Japan

    2001.04 - Now 

Professional Memberships

  • Japan Physical Scioety

      Domestic

  • 日本天文学会

      Domestic

  • Japan Physical Scioety

  • 日本天文学会

Job Career (off-campus)

  • Osaka Metropolitan University   Graduate School of Science, Department of Physics

    2022.04 - Now

  • Osaka Metropolitan University   Nambu Yoichiro Institute of Theoretical and Experimental Physics (NITEP)

    2022.04 - Now

  • 日本学術振興会 学術システム研究センター 主任研究員

    2019.04 - 2022.03

  • 日本学術振興会 学術システム研究センター 専門研究員

    2018.04 - 2019.03

  • 高エネルギー加速器研究機構 客員研究員

    2015.04 - 2016.03

  • Osaka City University   Graduate School of Science Mathematics and Physics Course

    2002.04 - 2022.03

  • Miyagi University of Education   Faculty of Education   Associated Professor

    1997.09 - 2002.03

  • University of Tokyo   Institute for Cosmic Ray Research   Assistant

    1993.04 - 1997.08

▼display all

Education

  • Osaka University   Physics division     Graduated/Completed

    1984.04 - 1988.03

  • Osaka University    

Papers

  • Overview of KAGRA: Data transfer and management

    Akutsu T.

    Progress of Theoretical and Experimental Physics   2023 ( 10 )   2023.10

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1093/ptep/ptad112

  • Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO-Virgo Observing Run O3a

    Abbott R.

    Astrophysical Journal   955 ( 2 )   2023.10( ISSN:0004637X

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/acd770

  • GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run

    R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, C. Adams, N. Adhikari, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, S. Akcay, T. Akutsu, S. Albanesi, A. Allocca, P. A. Altin, A. Amato, C. Anand, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, T. Andrade, N. Andres, T. Andrić, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, S. Appert, Koji Arai, Koya Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, M. Arogeti, S. M. Aronson, K. G. Arun, H. Asada, Y. Asali, G. Ashton, Y. Aso, M. Assiduo, S. M. Aston, P. Astone, F. Aubin, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, C. Badger, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, L. Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger

    Physical Review X   13 ( 4 )   2023.10( eISSN:2160-3308

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    Publishing type:Research paper (scientific journal)  

    The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the previous GWTC-2.1, we present candidate gravitational waves from compact binary coalescences during the second half of the third observing run (O3b) between 1 November 2019, 15∶00 Coordinated Universal Time (UTC) and 27 March 2020, 17∶00 UTC. There are 35 compact binary coalescence candidates identified by at least one of our search algorithms with a probability of astrophysical origin pastro>0.5. Of these, 18 were previously reported as low-latency public alerts, and 17 are reported here for the first time. Based upon estimates for the component masses, our O3b candidates with pastro>0.5 are consistent with gravitational-wave signals from binary black holes or neutron-star-black-hole binaries, and we identify none from binary neutron stars. However, from the gravitational-wave data alone, we are not able to measure matter effects that distinguish whether the binary components are neutron stars or black holes. The range of inferred component masses is similar to that found with previous catalogs, but the O3b candidates include the first confident observations of neutron-star-black-hole binaries. Including the 35 candidates from O3b in addition to those from GWTC-2.1, GWTC-3 contains 90 candidates found by our analysis with pastro>0.5 across the first three observing runs. These observations of compact binary coalescences present an unprecedented view of the properties of black holes and neutron stars.

    DOI: 10.1103/PhysRevX.13.041039

  • Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

    Abbott R.

    Astrophysical Journal, Supplement Series   267 ( 2 )   2023.08( ISSN:00670049

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4365/acdc9f

  • Development of advanced photon calibrator for Kamioka gravitational wave detector (KAGRA)

    Inoue Y.

    Review of Scientific Instruments   94 ( 7 )   2023.07( ISSN:00346748

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1063/5.0147888

  • Constraints on the Cosmic Expansion History from GWTC-3

    Abbott R.

    Astrophysical Journal   949 ( 2 )   2023.06( ISSN:0004637X

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/ac74bb

  • Noise subtraction from KAGRA O3GK data using Independent Component Analysis

    Abe H.

    Classical and Quantum Gravity   40 ( 8 )   2023.04( ISSN:02649381

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1088/1361-6382/acc0cb

  • Input optics systems of the KAGRA detector during O3GK

    Akutsu T.

    Progress of Theoretical and Experimental Physics   2023 ( 2 )   2023.02

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1093/ptep/ptac166

  • Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3

    Abbott R.

    Physical Review X   13 ( 1 )   2023.01

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevX.13.011048

  • Model-based Cross-correlation Search for Gravitational Waves from the Low-mass X-Ray Binary Scorpius X-1 in LIGO O3 Data

    Abbott R.

    Astrophysical Journal Letters   941 ( 2 )   2022.12( ISSN:20418205

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/2041-8213/aca1b0

  • All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data

    R. Abbott, H. Abe, F. Acernese, K. Ackley, N. Adhikari, R. X. Adhikari, V. K. Adkins, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, S. Albanesi, R. A. Alfaidi, A. Allocca, P. A. Altin, A. Amato, C. Anand, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, T. Andrade, N. Andres, M. Andrés-Carcasona, T. Andrić, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, T. Apostolatos, E. Z. Appavuravther, S. Appert, S. K. Apple, K. Arai, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, M. Arogeti, S. M. Aronson, H. Asada, Y. Asali, G. Ashton, Y. Aso, M. Assiduo, S. Assis De Souza Melo, S. M. Aston, P. Astone, F. Aubin, K. Aultoneal, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, C. Badger, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, J. Baird, R. Bajpai, T. Baka, M. Ball, G. Ballardin, S. W. Ballmer, A. Balsamo, G. Baltus, S. Banagiri, B. Banerjee, D. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, S. Basak, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, M. Bazzan

    Physical Review D   106 ( 10 )   2022.11( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    We present results of an all-sky search for continuous gravitational waves which can be produced by spinning neutron stars with an asymmetry around their rotation axis, using data from the third observing run of the Advanced LIGO and Advanced Virgo detectors. Four different analysis methods are used to search in a gravitational-wave frequency band from 10 to 2048 Hz and a first frequency derivative from -10-8 to 10-9 Hz/s. No statistically significant periodic gravitational-wave signal is observed by any of the four searches. As a result, upper limits on the gravitational-wave strain amplitude h0 are calculated. The best upper limits are obtained in the frequency range of 100 to 200 Hz and they are ∼1.1×10-25 at 95% confidence level. The minimum upper limit of 1.10×10-25 is achieved at a frequency 111.5 Hz. We also place constraints on the rates and abundances of nearby planetary- and asteroid-mass primordial black holes that could give rise to continuous gravitational-wave signals.

    DOI: 10.1103/PhysRevD.106.102008

  • Prevalence and Risk Factor Analysis of Post-Intensive Care Syndrome in Patients with COVID-19 Requiring Mechanical Ventilation: A Multicenter Prospective Observational Study

    Hatakeyama J.

    Journal of Clinical Medicine   11 ( 19 )   2022.10

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3390/jcm11195758

  • Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data

    R. Abbott, H. Abe, F. Acernese, K. Ackley, N. Adhikari, R. X. Adhikari, V. K. Adkins, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, S. Albanesi, R. A. Alfaidi, A. Allocca, P. A. Altin, A. Amato, C. Anand, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, T. Andrade, N. Andres, M. Andrés-Carcasona, T. Andrić, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, T. Apostolatos, E. Z. Appavuravther, S. Appert, S. K. Apple, K. Arai, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, M. Arogeti, S. M. Aronson, H. Asada, Y. Asali, G. Ashton, Y. Aso, M. Assiduo, S. Assis de Souza Melo, S. M. Aston, P. Astone, F. Aubin, K. AultONeal, C. Austin, S. Babak, F. Badaracco, M. K. M. Bader, C. Badger, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, J. Baird, R. Bajpai, T. Baka, M. Ball, G. Ballardin, S. W. Ballmer, A. Balsamo, G. Baltus, S. Banagiri, B. Banerjee, D. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, S. Basak, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, M. Bazzan, B. R. Becher, B. Bécsy, V. M. Bedakihale, F. Beirnaert, M. Bejger, I. Belahcene, V. Benedetto, D. Beniwal, M. G. Benjamin, T. F. Bennett, J. D. Bentley, M. BenYaala, S. Bera, M. Berbel, F. Bergamin, B. K. Berger, S. Bernuzzi, D. Bersanetti, A. Bertolini, J. Betzwieser, D. Beveridge, R. Bhandare, A. V. Bhandari, U. Bhardwaj, R. Bhatt, D. Bhattacharjee, S. Bhaumik, A. Bianchi, I. A. Bilenko, G. Billingsley, S. Bini, R. Birney, O. Birnholtz, S. Biscans, M. Bischi, S. Biscoveanu, A. Bisht, B. Biswas, M. Bitossi, M.-A. Bizouard, J. K. Blackburn, C. D. Blair, D. G. Blair, R. M. Blair, F. Bobba, N. Bode, M. Boër, G. Bogaert, M. Boldrini, G. N. Bolingbroke, L. D. Bonavena, F. Bondu, E. Bonilla, R. Bonnand, P. Booker, B. A. Boom, R. Bork, V. Boschi, N. Bose, S. Bose, V. Bossilkov, V. Boudart, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. R. Brady, A. Bramley, A. Branch, M. Branchesi, J. E. Brau, M. Breschi, T. Briant, J. H. Briggs, A. Brillet, M. Brinkmann, P. Brockill, A. F. Brooks, J. Brooks, D. D. Brown, S. Brunett, G. Bruno, R. Bruntz, J. Bryant, F. Bucci, T. Bulik, H. J. Bulten, A. Buonanno, K. Burtnyk, R. Buscicchio, D. Buskulic, C. Buy, R. L. Byer, G. S. Cabourn Davies, G. Cabras, R. Cabrita, L. Cadonati, M. Caesar, G. Cagnoli, C. Cahillane, J. Calderón Bustillo, J. D. Callaghan, T. A. Callister, E. Calloni, J. Cameron, J. B. Camp, M. Canepa, S. Canevarolo, M. Cannavacciuolo, K. C. Cannon, H. Cao, Z. Cao, E. Capocasa, E. Capote, G. Carapella, F. Carbognani, M. Carlassara, J. B. Carlin, M. F. Carney, M. Carpinelli, G. Carrillo, G. Carullo, T. L. Carver, J. Casanueva Diaz, C. Casentini, G. Castaldi, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, G. Cella, P. Cerdá-Durán, E. Cesarini, W. Chaibi, S. Chalathadka Subrahmanya, E. Champion, C.-H. Chan, C. Chan, C. L. Chan, K. Chan, M. Chan, K. Chandra, I. P. Chang, P. Chanial, S. Chao, C. Chapman-Bird, P. Charlton, E. A. Chase, E. Chassande-Mottin, C. Chatterjee, Debarati Chatterjee, Deep Chatterjee, M. Chaturvedi, S. Chaty, C. Chen, D. Chen, H. Y. Chen, J. Chen, K. Chen, X. Chen, Y.-B. Chen, Y.-R. Chen, Z. Chen, H. Cheng, C. K. Cheong, H. Y. Cheung, H. Y. Chia, F. Chiadini, C-Y. Chiang, G. Chiarini, R. Chierici, A. Chincarini, M. L. Chiofalo, A. Chiummo, R. K. Choudhary, S. Choudhary, N. Christensen, Q. Chu, Y-K. Chu, S. S. Y. Chua, K. W. Chung, G. Ciani, P. Ciecielag, M. Cieślar, M. Cifaldi, A. A. Ciobanu, R. Ciolfi, F. Cipriano, F. Clara, J. A. Clark, P. Clearwater, S. Clesse, F. Cleva, E. Coccia, E. Codazzo, P.-F. Cohadon, D. E. Cohen, M. Colleoni, C. G. Collette, A. Colombo, M. Colpi, C. M. Compton, M. Constancio, L. Conti, S. J. Cooper, P. Corban, T. R. Corbitt, I. Cordero-Carrión, S. Corezzi, K. R. Corley, N. J. Cornish, D. Corre, A. Corsi, S. Cortese, C. A. Costa, R. Cotesta, R. Cottingham, M. W. Coughlin, J.-P. Coulon, S. T. Countryman, B. Cousins, P. Couvares, D. M. Coward, M. J. Cowart, D. C. Coyne, R. Coyne, J. D. E. Creighton, T. D. Creighton, A. W. Criswell, M. Croquette, S. G. Crowder, J. R. Cudell, T. J. Cullen, A. Cumming, R. Cummings, L. Cunningham, E. Cuoco, M. Curyło, P. Dabadie, T. Dal Canton, S. Dall’Osso, G. Dálya, A. Dana, B. D’Angelo, S. Danilishin, S. D’Antonio, K. Danzmann, C. Darsow-Fromm, A. Dasgupta, L. E. H. Datrier, Sayak Datta, Sayantani Datta, V. Dattilo, I. Dave, M. Davier, D. Davis, M. C. Davis, E. J. Daw, R. Dean, D. DeBra, M. Deenadayalan, J. Degallaix, M. De Laurentis, S. Deléglise, V. Del Favero, F. De Lillo, N. De Lillo, D. Dell’Aquila, W. Del Pozzo, L. M. DeMarchi, F. De Matteis, V. D’Emilio, N. Demos, T. Dent, A. Depasse, R. De Pietri, R. De Rosa, C. De Rossi, R. DeSalvo, R. De Simone, S. Dhurandhar, M. C. Díaz, N. A. Didio, T. Dietrich, L. Di Fiore, C. Di Fronzo, C. Di Giorgio, F. Di Giovanni, M. Di Giovanni, T. Di Girolamo, A. Di Lieto, A. Di Michele, B. Ding, S. Di Pace, I. Di Palma, F. Di Renzo, A. K. Divakarla, A. Dmitriev, Z. Doctor, L. Donahue, L. D’Onofrio, F. Donovan, K. L. Dooley, S. Doravari, M. Drago, J. C. Driggers, Y. Drori, J.-G. Ducoin, P. Dupej, U. Dupletsa, O. Durante, D. D’Urso, P.-A. Duverne, S. E. Dwyer, C. Eassa, P. J. Easter, M. Ebersold, T. Eckhardt, G. Eddolls, B. Edelman, T. B. Edo, O. Edy, A. Effler, S. Eguchi, J. Eichholz, S. S. Eikenberry, M. Eisenmann, R. A. Eisenstein, A. Ejlli, E. Engelby, Y. Enomoto, L. Errico, R. C. Essick, H. Estellés, D. Estevez, Z. Etienne, T. Etzel, M. Evans, T. M. Evans, T. Evstafyeva, B. E. Ewing, F. Fabrizi, F. Faedi, V. Fafone, H. Fair, S. Fairhurst, P. C. Fan, A. M. Farah, S. Farinon, B. Farr, W. M. Farr, E. J. Fauchon-Jones, G. Favaro, M. Favata, M. Fays, M. Fazio, J. Feicht, M. M. Fejer, E. Fenyvesi, D. L. Ferguson, A. Fernandez-Galiana, I. Ferrante, T. A. Ferreira, F. Fidecaro, P. Figura, A. Fiori, I. Fiori, M. Fishbach, R. P. Fisher, R. Fittipaldi, V. Fiumara, R. Flaminio, E. Floden, H. K. Fong, J. A. Font, B. Fornal, P. W. F. Forsyth, A. Franke, S. Frasca, F. Frasconi, J. P. Freed, Z. Frei, A. Freise, O. Freitas, R. Frey, P. Fritschel, V. V. Frolov, G. G. Fronzé, Y. Fujii, Y. Fujikawa, Y. Fujimoto, P. Fulda, M. Fyffe, H. A. Gabbard, B. U. Gadre, J. R. Gair, J. Gais, S. Galaudage, R. Gamba, D. Ganapathy, A. Ganguly, D. Gao, S. G. Gaonkar, B. Garaventa, C. García Núñez, C. García-Quirós, F. Garufi, B. Gateley, V. Gayathri, G.-G. Ge, G. Gemme, A. Gennai, J. George, O. Gerberding, L. Gergely, P. Gewecke, S. Ghonge, Abhirup Ghosh, Archisman Ghosh, Shaon Ghosh, Shrobana Ghosh, Tathagata Ghosh, B. Giacomazzo, L. Giacoppo, J. A. Giaime, K. D. Giardina, D. R. Gibson, C. Gier, M. Giesler, P. Giri, F. Gissi, S. Gkaitatzis, J. Glanzer, A. E. Gleckl, P. Godwin, E. Goetz, R. Goetz, N. Gohlke, J. Golomb, B. Goncharov, G. González, M. Gosselin, R. Gouaty, D. W. Gould, S. Goyal, B. Grace, A. Grado, V. Graham, M. Granata, V. Granata, A. Grant, S. Gras, P. Grassia, C. Gray, R. Gray, G. Greco, A. C. Green, R. Green, A. M. Gretarsson, E. M. Gretarsson, D. Griffith, W. L. Griffiths, H. L. Griggs, G. Grignani, A. Grimaldi, E. Grimes, S. J. Grimm, H. Grote, S. Grunewald, P. Gruning, A. S. Gruson, D. Guerra, G. M. Guidi, A. R. Guimaraes, G. Guixé, H. K. Gulati, A. M. Gunny, H.-K. Guo, Y. Guo, Anchal Gupta, Anuradha Gupta, I. M. Gupta, P. Gupta, S. K. Gupta, R. Gustafson, F. Guzman, S. Ha, I. P. W. Hadiputrawan, L. Haegel, S. Haino, O. Halim, E. D. Hall, E. Z. Hamilton, G. Hammond, W.-B. Han, M. Haney, J. Hanks, C. Hanna, M. D. Hannam, O. Hannuksela, H. Hansen, T. J. Hansen, J. Hanson, T. Harder, K. Haris, J. Harms, G. M. Harry, I. W. Harry, D. Hartwig, K. Hasegawa, B. Haskell, C.-J. Haster, J. S. Hathaway, K. Hattori, K. Haughian, H. Hayakawa, K. Hayama, F. J. Hayes, J. Healy, A. Heidmann, A. Heidt, M. C. Heintze, J. Heinze, J. Heinzel, H. Heitmann, F. Hellman, P. Hello, A. F. Helmling-Cornell, G. 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Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

    Physical Review D   106 ( 6 )   2022.09( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    Results are presented for a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to allow for spin wandering. This search improves on previous HMM-based searches of Laser Interferometer Gravitational-Wave Observatory data by including the orbital period in the search template grid, and by analyzing data from the latest (third) observing run. In the frequency range searched, from 60 to 500 Hz, we find no evidence of gravitational radiation. This is the most sensitive search for Scorpius X-1 using a HMM to date. For the most sensitive subband, starting at 256.06 Hz, we report an upper limit on gravitational wave strain (at 95% confidence) of h095%=6.16×10-26, assuming the orbital inclination angle takes its electromagnetically restricted value ι=44°. The upper limits on gravitational wave strain reported here are on average a factor of ∼3 lower than in the second observing run HMM search. This is the first Scorpius X-1 HMM search with upper limits that reach below the indirect torque-balance limit for certain subbands, assuming ι=44°.

    DOI: 10.1103/physrevd.106.062002

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.106.062002/fulltext

  • Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data

    Abbott R.

    Physical Review D   106 ( 4 )   2022.08( ISSN:24700010

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.106.042003

  • Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs

    Abbott R.

    Astrophysical Journal   935 ( 1 )   2022.08( ISSN:0004637X

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/ac6acf

  • Characteristics of colorectal neuroendocrine tumors in patients prospectively enrolled in a Japanese multicenter study: a first report from the C-NET STUDY

    Sekiguchi M.

    Journal of Gastroenterology   57 ( 8 )   547 - 558   2022.08( ISSN:09441174

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1007/s00535-022-01877-5

  • Charge-changing cross sections for Ca 42-51 and effect of charged-particle evaporation induced by neutron-removal reactions

    Tanaka M.

    Physical Review C   106 ( 1 )   2022.07( ISSN:24699985

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevC.106.014617

  • Performance of the KAGRA detector during the first joint observation with GEO 600 (O3GK)

    H Abe, R X Adhikari, T Akutsu, M Ando, A Araya, N Aritomi, H Asada, Y Aso, S Bae, Y Bae, R Bajpai, S W Ballmer, K Cannon, Z Cao, E Capocasa, M Chan, C Chen, D Chen, K Chen, Y Chen, C-Y Chiang, Y-K Chu, J C Driggers, S E Dwyer, A Effler, S Eguchi, M Eisenmann, Y Enomoto, R Flaminio, H K Fong, V V Frolov, Y Fujii, Y Fujikawa, Y Fujimoto, M Fukushima, D Gao, G-G Ge, S Ha, I P W Hadiputrawan, S Haino, W-B Han, K Hasegawa, K Hattori, H Hayakawa, K Hayama, Y Himemoto, N Hirata, C Hirose, T-C Ho, B-H Hsieh, H-F Hsieh, C Hsiung, H-Y Huang, P Huang, Y-C Huang, Y-J Huang, D C Y Hui, S Ide, B Ikenoue, K Inayoshi, Y Inoue, K Ito, Y Itoh, K Izumi, C Jeon, H-B Jin, K Jung, P Jung, K Kaihotsu, T Kajita, M Kakizaki, M Kamiizumi, N Kanda, T Kato, K Kawabe, K Kawaguchi, C Kim, J Kim, J C Kim, Y-M Kim, N Kimura, Y Kobayashi, K Kohri, K Kokeyama, A K H Kong, N Koyama, C Kozakai, J Kume, Y Kuromiya, S Kuroyanagi, K Kwak, E Lee, H W Lee, R Lee, M Leonardi, K L Li, P Li, L C-C Lin, C-Y Lin, E T Lin, F-K Lin, F-L Lin, H L Lin, G C Liu, L-W Luo, M Ma’arif, E Majorana, Y Michimura, N Mio, O Miyakawa, K Miyo, S Miyoki, Y Mori, S Morisaki, N Morisue, Y Moriwaki, A Mullavey, K Nagano, K Nakamura, H Nakano, M Nakano, Y Nakayama, T Narikawa, L Naticchioni, L Nguyen Quynh, W-T Ni, T Nishimoto, A Nishizawa, S Nozaki, Y Obayashi, Y Obuchi, W Ogaki, J J Oh, K Oh, M Ohashi, T Ohashi, M Ohkawa, H Ohta, Y Okutani, K Oohara, S Oshino, S Otabe, K-C Pan, A Parisi, J Park, F E Peña Arellano, S Saha, S Saito, Y Saito, K Sakai, T Sawada, Y Sekiguchi, L Shao, Y Shikano, H Shimizu, R Shimizu, K Shimode, H Shinkai, T Shishido, A Shoda, K Somiya, I Song, R Sugimoto, J Suresh, T Suzuki, T Suzuki, T Suzuki, H Tagoshi, H Takahashi, R Takahashi, S Takano, H Takeda, M Takeda, M Tamaki, K Tanaka, T Tanaka, T Tanaka, S Tanioka, A Taruya, T Tomaru, T Tomura, L Trozzo, T Tsang, J-S Tsao, S Tsuchida, T Tsutsui, T Tsuzuki, D Tuyenbayev, N Uchikata, T Uchiyama, A Ueda, T Uehara, K Ueno, G Ueshima, F Uraguchi, T Ushiba, M H P M van Putten, J Wang, T Washimi, C Wu, H Wu, T Yamada, K Yamamoto, T Yamamoto, K Yamashita, R Yamazaki, Y Yang, S-W Yeh, J Yokoyama, T Yokozawa, T Yoshioka, H Yuzurihara, S Zeidler, M Zhan, H Zhang, Y Zhao, Z-H Zhu

    Progress of Theoretical and Experimental Physics   2022.06( eISSN:2050-3911

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    Publishing type:Research paper (scientific journal)  

    Abstract

    KAGRA, the kilometer-scale underground gravitational-wave detector, is located at Kamioka, Japan. In April 2020, an astrophysics observation was performed at the KAGRA detector in combination with the GEO 600 detector; this observation operation is called O3GK. The optical configuration in O3GK is based on a power-recycled Fabry–Pérot–Michelson interferometer; all the mirrors were set at room temperature. The duty factor of the operation was approximately 53%, and the displacement sensitivity was approximately 1 × 10−18 ${\rm m}/\sqrt{\rm {Hz } }$ at 250 Hz. The binary-neutron-star (BNS) inspiral range was about 0.6 Mpc. The contributions of various noise sources to the sensitivity of O3GK were investigated to understand how the observation range could be improved; this study is called a “noise budget”. According to our noise budget, the measured sensitivity could be approximated by adding up the effect of each noise. The sensitivity was dominated by noise from the sensors used for local controls of the vibration isolation systems, acoustic noise, shot noise, and laser frequency noise. Further, other noise sources that did not limit the sensitivity were investigated. This paper provides a detailed account of the KAGRA detector in O3GK, including interferometer configuration, status, and noise budget. In addition, strategies for future sensitivity improvements, such as hardware upgrades, are discussed.

    DOI: 10.1093/ptep/ptac093

  • First joint observation by the underground gravitational-wave detector KAGRA with GEO 600

    R Abbott, H Abe, F Acernese, K Ackley, N Adhikari, R X Adhikari, V K Adkins, V B Adya, C Affeldt, D Agarwal, M Agathos, K Agatsuma, N Aggarwal, O D Aguiar, L Aiello, A Ain, P Ajith, T Akutsu, S Albanesi, R A Alfaidi, A Allocca, P A Altin, A Amato, C Anand, S Anand, A Ananyeva, S B Anderson, W G Anderson, M Ando, T Andrade, N Andres, M Andrés-Carcasona, T Andrić, S V Angelova, S Ansoldi, J M Antelis, S Antier, T Apostolatos, E Z Appavuravther, S Appert, S K Apple, K Arai, A Araya, M C Araya, J S Areeda, M Arène, N Aritomi, N Arnaud, M Arogeti, S M Aronson, K G Arun, H Asada, Y Asali, G Ashton, Y Aso, M Assiduo, S Assis de Souza Melo, S M Aston, P Astone, F Aubin, K AultONeal, C Austin, S Babak, F Badaracco, M K M Bader, C Badger, S Bae, Y Bae, A M Baer, S Bagnasco, Y Bai, J Baird, R Bajpai, T Baka, M Ball, G Ballardin, S W Ballmer, A Balsamo, G Baltus, S Banagiri, B Banerjee, D Bankar, J C Barayoga, C Barbieri, B C Barish, D Barker, P Barneo, F Barone, B Barr, L Barsotti, M Barsuglia, D Barta, J Bartlett, M A Barton, I Bartos, S Basak, R Bassiri, A Basti, M Bawaj, J C Bayley, M Bazzan, B R Becher, B Bécsy, V M Bedakihale, F Beirnaert, M Bejger, I Belahcene, V Benedetto, D Beniwal, M G Benjamin, T F Bennett, J D Bentley, M BenYaala, S Bera, M Berbel, F Bergamin, B K Berger, S Bernuzzi, C P L Berry, D Bersanetti, A Bertolini, J Betzwieser, D Beveridge, R Bhandare, A V Bhandari, U Bhardwaj, R Bhatt, D Bhattacharjee, S Bhaumik, A Bianchi, I A Bilenko, G Billingsley, S Bini, R Birney, O Birnholtz, S Biscans, M Bischi, S Biscoveanu, A Bisht, B Biswas, M Bitossi, M-A Bizouard, J K Blackburn, C D Blair, D G Blair, R M Blair, F Bobba, N Bode, M Boër, G Bogaert, M Boldrini, G N Bolingbroke, L D Bonavena, F Bondu, E Bonilla, R Bonnand, P Booker, B A Boom, R Bork, V Boschi, N Bose, S Bose, V Bossilkov, V Boudart, Y Bouffanais, A Bozzi, C Bradaschia, P R Brady, A Bramley, A Branch, M Branchesi, J E Brau, M Breschi, T Briant, J H Briggs, A Brillet, M Brinkmann, P Brockill, A F Brooks, J Brooks, D D Brown, S Brunett, G Bruno, R Bruntz, J Bryant, F Bucci, T Bulik, H J Bulten, A Buonanno, K Burtnyk, R Buscicchio, D Buskulic, C Buy, R L Byer, G S Cabourn Davies, G Cabras, R Cabrita, L Cadonati, M Caesar, G Cagnoli, C Cahillane, J Calderón Bustillo, J D Callaghan, T A Callister, E Calloni, J Cameron, J B Camp, M Canepa, S Canevarolo, M Cannavacciuolo, K C Cannon, H Cao, Z Cao, E Capocasa, E Capote, G Carapella, F Carbognani, M Carlassara, J B Carlin, M F Carney, M Carpinelli, G Carrillo, G Carullo, T L Carver, J Casanueva Diaz, C Casentini, G Castaldi, S Caudill, M Cavaglià, F Cavalier, R Cavalieri, G Cella, P Cerdá-Durán, E Cesarini, W Chaibi, S Chalathadka Subrahmanya, E Champion, C-H Chan, C Chan, C L Chan, K Chan, M Chan, K Chandra, I P Chang, P Chanial, S Chao, C Chapman-Bird, P Charlton, E A Chase, E Chassande-Mottin, C Chatterjee, Debarati Chatterjee, Deep Chatterjee, M Chaturvedi, S Chaty, C Chen, D Chen, H Y Chen, J Chen, K Chen, X Chen, Y-B Chen, Y-R Chen, Z Chen, H Cheng, C K Cheong, H Y Cheung, H Y Chia, F Chiadini, C-Y Chiang, G Chiarini, R Chierici, A Chincarini, M L Chiofalo, A Chiummo, R K Choudhary, S Choudhary, N Christensen, Q Chu, Y-K Chu, S S Y Chua, K W Chung, G Ciani, P Ciecielag, M Cieślar, M Cifaldi, A A Ciobanu, R Ciolfi, F Cipriano, F Clara, J A Clark, P Clearwater, S Clesse, F Cleva, E Coccia, E Codazzo, P-F Cohadon, D E Cohen, M Colleoni, C G Collette, A Colombo, M Colpi, C M Compton, M Constancio Jr., L Conti, S J Cooper, P Corban, T R Corbitt, I Cordero-Carrión, S Corezzi, K R Corley, N J Cornish, D Corre, A Corsi, S Cortese, C A Costa, R Cotesta, R Cottingham, M W Coughlin, J-P Coulon, S T Countryman, B Cousins, P Couvares, D M Coward, M J Cowart, D C Coyne, R Coyne, J D E Creighton, T D Creighton, A W Criswell, M Croquette, S G Crowder, J R Cudell, T J Cullen, A Cumming, R Cummings, L Cunningham, E Cuoco, M Curyło, P Dabadie, T Dal Canton, S Dall’Osso, G Dálya, A Dana, B D’Angelo, S Danilishin, S D’Antonio, K Danzmann, C Darsow-Fromm, A Dasgupta, L E H Datrier, Sayak Datta, Sayantani Datta, V Dattilo, I Dave, M Davier, D Davis, M C Davis, E J Daw, R Dean, D DeBra, M Deenadayalan, J Degallaix, M De Laurentis, S Deléglise, V Del Favero, F De Lillo, N De Lillo, D Dell’Aquila, W Del Pozzo, L M DeMarchi, F De Matteis, V D’Emilio, N Demos, T Dent, A Depasse, R De Pietri, R De Rosa, C De Rossi, R DeSalvo, R De Simone, S Dhurandhar, M C Díaz, N A Didio, T Dietrich, L Di Fiore, C Di Fronzo, C Di Giorgio, F Di Giovanni, M Di Giovanni, T Di Girolamo, A Di Lieto, A Di Michele, B Ding, S Di Pace, I Di Palma, F Di Renzo, A K Divakarla, A Dmitriev, Z Doctor, L Donahue, L D’Onofrio, F Donovan, K L Dooley, S Doravari, M Drago, J C Driggers, Y Drori, J-G Ducoin, P Dupej, U Dupletsa, O Durante, D D’Urso, P-A Duverne, S E Dwyer, C Eassa, P J Easter, M Ebersold, T Eckhardt, G Eddolls, B Edelman, T B Edo, O Edy, A Effler, S Eguchi, J Eichholz, S S Eikenberry, M Eisenmann, R A Eisenstein, A Ejlli, E Engelby, Y Enomoto, L Errico, R C Essick, H Estellés, D Estevez, Z Etienne, T Etzel, M Evans, T M Evans, T Evstafyeva, B E Ewing, F Fabrizi, F Faedi, V Fafone, H Fair, S Fairhurst, P C Fan, A M Farah, S Farinon, B Farr, W M Farr, E J Fauchon-Jones, G Favaro, M Favata, M Fays, M Fazio, J Feicht, M M Fejer, E Fenyvesi, D L Ferguson, A Fernandez-Galiana, I Ferrante, T A Ferreira, F Fidecaro, P Figura, A Fiori, I Fiori, M Fishbach, R P Fisher, R Fittipaldi, V Fiumara, R Flaminio, E Floden, H K Fong, J A Font, B Fornal, P W F Forsyth, A Franke, S Frasca, F Frasconi, J P Freed, Z Frei, A Freise, O Freitas, R Frey, V V Frolov, G G Fronzé, Y Fujii, Y Fujikawa, Y Fujimoto, P Fulda, M Fyffe, H A Gabbard, W E Gabella, B U Gadre, J R Gair, J Gais, S Galaudage, R Gamba, D Ganapathy, A Ganguly, D Gao, S G Gaonkar, B Garaventa, C García Núñez, C García-Quirós, F Garufi, B Gateley, V Gayathri, G-G Ge, G Gemme, A Gennai, J George, O Gerberding, L Gergely, P Gewecke, S Ghonge, Abhirup Ghosh, Archisman Ghosh, Shaon Ghosh, Shrobana Ghosh, Tathagata Ghosh, B Giacomazzo, L Giacoppo, J A Giaime, K D Giardina, D R Gibson, C Gier, M Giesler, P Giri, F Gissi, S Gkaitatzis, J Glanzer, A E Gleckl, P Godwin, E Goetz, R Goetz, N Gohlke, J Golomb, B Goncharov, G González, M Gosselin, R Gouaty, D W Gould, S Goyal, B Grace, A Grado, V Graham, M Granata, V Granata, A Grant, S Gras, P Grassia, C Gray, R Gray, G Greco, A C Green, R Green, A M Gretarsson, E M Gretarsson, D Griffith, W L Griffiths, H L Griggs, G Grignani, A Grimaldi, E Grimes, S J Grimm, H Grote, S Grunewald, P Gruning, A S Gruson, D Guerra, G M Guidi, A R Guimaraes, G Guixé, H K Gulati, A M Gunny, H-K Guo, Y Guo, Anchal Gupta, Anuradha Gupta, I M Gupta, P Gupta, S K Gupta, R Gustafson, F Guzman, S Ha, I P W Hadiputrawan, L Haegel, S Haino, O Halim, E D Hall, E Z Hamilton, G Hammond, W-B Han, M Haney, J Hanks, C Hanna, M D Hannam, O Hannuksela, H Hansen, T J Hansen, J Hanson, T Harder, K Haris, J Harms, G M Harry, I W Harry, D Hartwig, K Hasegawa, B Haskell, C-J Haster, J S Hathaway, K Hattori, K Haughian, H Hayakawa, K Hayama, F J Hayes, J Healy, A Heidmann, A Heidt, M C Heintze, J Heinze, J Heinzel, H Heitmann, F Hellman, P Hello, A F Helmling-Cornell, G Hemming, M Hendry, I S Heng, E Hennes, J Hennig, M H Hennig, C Henshaw, A G Hernandez, F Hernandez Vivanco, M Heurs, A L Hewitt, S Higginbotham, S Hild, P Hill, Y Himemoto, A S Hines, N Hirata, C Hirose, T-C Ho, S Hochheim, D Hofman, J N Hohmann, D G Holcomb, N A Holland, I J Hollows, Z J Holmes, K Holt, D E Holz, Q Hong, J Hough, S Hourihane, E J Howell, C G Hoy, D Hoyland, A Hreibi, B-H Hsieh, H-F Hsieh, C Hsiung, Y Hsu, H-Y Huang, P Huang, Y-C Huang, Y-J Huang, Yiting Huang, Yiwen Huang, M T Hübner, A D Huddart, B Hughey, D C Y Hui, V Hui, S Husa, S H Huttner, R Huxford, T Huynh-Dinh, S Ide, B Idzkowski, A Iess, K Inayoshi, Y Inoue, P Iosif, M Isi, K Isleif, K Ito, Y Itoh, B R Iyer, V JaberianHamedan, T Jacqmin, P-E Jacquet, S J Jadhav, S P Jadhav, T Jain, A L James, A Z Jan, K Jani, J Janquart, K Janssens, N N Janthalur, P Jaranowski, D Jariwala, R Jaume, A C Jenkins, K Jenner, C Jeon, W Jia, J Jiang, H-B Jin, G R Johns, R Johnston, A W Jones, D I Jones, P Jones, R Jones, P Joshi, L Ju, A Jue, P Jung, K Jung, J Junker, V Juste, K Kaihotsu, T Kajita, M Kakizaki, C V Kalaghatgi, V Kalogera, B Kamai, M Kamiizumi, N Kanda, S Kandhasamy, G Kang, J B Kanner, Y Kao, S J Kapadia, D P Kapasi, C Karathanasis, S Karki, R Kashyap, M Kasprzack, W Kastaun, T Kato, S Katsanevas, E Katsavounidis, W Katzman, T Kaur, K Kawabe, K Kawaguchi, F Kéfélian, D Keitel, J S Key, S Khadka, F Y Khalili, S Khan, T Khanam, E A Khazanov, N Khetan, M Khursheed, N Kijbunchoo, A Kim, C Kim, J C Kim, J Kim, K Kim, W S Kim, Y-M Kim, C Kimball, N Kimura, M Kinley-Hanlon, R Kirchhoff, J S Kissel, S Klimenko, T Klinger, A M Knee, T D Knowles, N Knust, E Knyazev, Y Kobayashi, P Koch, G Koekoek, K Kohri, K Kokeyama, S Koley, P Kolitsidou, M Kolstein, K Komori, V Kondrashov, A K H Kong, A Kontos, N Koper, M Korobko, M Kovalam, N Koyama, D B Kozak, C Kozakai, V Kringel, N V Krishnendu, A Królak, G Kuehn, F Kuei, P Kuijer, S Kulkarni, A Kumar, Prayush Kumar, Rahul Kumar, Rakesh Kumar, J Kume, K Kuns, Y Kuromiya, S Kuroyanagi, K Kwak, G Lacaille, P Lagabbe, D Laghi, E Lalande, M Lalleman, T L Lam, A Lamberts, M Landry, B B Lane, R N Lang, J Lange, B Lantz, I La Rosa, A Lartaux-Vollard, P D Lasky, M Laxen, A Lazzarini, C Lazzaro, P Leaci, S Leavey, S LeBohec, Y K Lecoeuche, E Lee, H M Lee, H W Lee, K Lee, R Lee, I N Legred, J Lehmann, A Lemaître, M Lenti, M Leonardi, E Leonova, N Leroy, N Letendre, C Levesque, Y Levin, J N Leviton, K Leyde, A K Y Li, B Li, J Li, K L Li, P Li, T G F Li, X Li, C-Y Lin, E T Lin, F-K Lin, F-L Lin, H L Lin, L C-C Lin, F Linde, S D Linker, J N Linley, T B Littenberg, G C Liu, J Liu, K Liu, X Liu, F Llamas, R K L Lo, T Lo, L T London, A Longo, D Lopez, M Lopez Portilla, M Lorenzini, V Loriette, M Lormand, G Losurdo, T P Lott, J D Lough, C 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    Progress of Theoretical and Experimental Physics   2022 ( 6 )   2022.06( eISSN:2050-3911

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    Publishing type:Research paper (scientific journal)  

    Abstract

    We report the results of the first joint observation of the KAGRA detector with GEO 600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with 3 km arms, located in Kamioka, Gifu, Japan. GEO 600 is a British–German laser interferometer with 600 m arms, located near Hannover, Germany. GEO 600 and KAGRA performed a joint observing run from April 7 to 20, 2020. We present the results of the joint analysis of the GEO–KAGRA data for transient gravitational-wave signals, including the coalescence of neutron-star binaries and generic unmodeled transients. We also perform dedicated searches for binary coalescence signals and generic transients associated with gamma-ray burst events observed during the joint run. No gravitational-wave events were identified. We evaluate the minimum detectable amplitude for various types of transient signals and the spacetime volume for which the network is sensitive to binary neutron-star coalescences. We also place lower limits on the distances to the gamma-ray bursts analyzed based on the non-detection of an associated gravitational-wave signal for several signal models, including binary coalescences. These analyses demonstrate the feasibility and utility of KAGRA as a member of the global gravitational-wave detector network.

    DOI: 10.1093/ptep/ptac073

    Other URL: https://academic.oup.com/ptep/article-pdf/2022/6/063F01/43989382/ptac073.pdf

  • All-sky, all-frequency directional search for persistent gravitational waves from Advanced LIGO’s and Advanced Virgo’s first three observing runs

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Yamamoto, Kazuhiro Yamamoto, Kohei Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, L. Yang, Y. Yang, Yang Yang, Z. Yang, M. J. Yap, D. W. Yeeles, A. B. Yelikar, M. Ying, K. Yokogawa, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, M. E. Zucker, J. Zweizig

    Physical Review D   105 ( 12 )   2022.06( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    We present the first results from an all-sky all-frequency (ASAF) search for an anisotropic stochastic gravitational-wave background using the data from the first three observing runs of the Advanced LIGO and Advanced Virgo detectors. Upper limit maps on broadband anisotropies of a persistent stochastic background were published for all observing runs of the LIGO-Virgo detectors. However, a broadband analysis is likely to miss narrowband signals as the signal-to-noise ratio of a narrowband signal can be significantly reduced when combined with detector output from other frequencies. Data folding and the computationally efficient analysis pipeline, PyStoch, enable us to perform the radiometer map-making at every frequency bin. We perform the search at 3072 HEALPix equal area pixels uniformly tiling the sky and in every frequency bin of width 1/32 Hz in the range 20-1726 Hz, except for bins that are likely to contain instrumental artefacts and hence are notched. We do not find any statistically significant evidence for the existence of narrowband gravitational-wave signals in the analyzed frequency bins. Therefore, we place 95% confidence upper limits on the gravitational-wave strain for each pixel-frequency pair, the limits are in the range (0.030-9.6)×10-24. In addition, we outline a method to identify candidate pixel-frequency pairs that could be followed up by a more sensitive (and potentially computationally expensive) search, e.g., a matched-filtering-based analysis, to look for fainter nearly monochromatic coherent signals. The ASAF analysis is inherently independent of models describing any spectral or spatial distribution of power. We demonstrate that the ASAF results can be appropriately combined over frequencies and sky directions to successfully recover the broadband directional and isotropic results.

    DOI: 10.1103/physrevd.105.122001

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.105.122001/fulltext

  • Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run

    Abbott R.

    Astrophysical Journal   932 ( 2 )   2022.06( ISSN:0004637X

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/ac6ad0

  • All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data

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Riemenschneider, K. Riles, S. Rinaldi, K. Rink, N. A. Robertson, R. Robie, F. Robinet, A. Rocchi, S. Rodriguez, L. Rolland, J. G. Rollins, M. Romanelli, R. Romano, C. L. Romel, A. Romero, I. M. Romero-Shaw, J. H. Romie, S. Ronchini, L. Rosa, C. A. Rose, D. Rosińska, M. P. Ross, S. Rowan, S. J. Rowlinson, S. Roy, Santosh Roy, Soumen Roy, D. Rozza, P. Ruggi, K. Ruiz-Rocha, K. Ryan, S. Sachdev, T. Sadecki, J. Sadiq, S. Saha, Y. Saito, K. Sakai, M. Sakellariadou, S. Sakon, O. S. Salafia, F. Salces-Carcoba, L. Salconi, M. Saleem, F. Salemi, A. Samajdar, E. J. Sanchez, J. H. Sanchez, L. E. Sanchez, N. Sanchis-Gual, J. R. Sanders, A. Sanuy, T. R. Saravanan, N. Sarin, B. Sassolas, H. Satari, O. Sauter, R. L. Savage, V. Savant, T. Sawada, H. L. Sawant, S. Sayah, D. Schaetzl, M. Scheel, J. Scheuer, M. G. Schiworski, P. Schmidt, S. Schmidt, R. Schnabel, M. Schneewind, R. M. S. Schofield, A. Schönbeck, B. W. Schulte, B. F. Schutz, E. Schwartz, J. Scott, S. M. Scott, M. Seglar-Arroyo, Y. Sekiguchi, D. Sellers, A. S. Sengupta, D. Sentenac, E. G. Seo, V. Sequino, A. Sergeev, Y. Setyawati, T. Shaffer, M. S. Shahriar, M. A. Shaikh, B. Shams, L. Shao, A. Sharma, P. Sharma, P. Shawhan, N. S. Shcheblanov, A. Sheela, Y. Shikano, M. Shikauchi, H. Shimizu, K. Shimode, H. Shinkai, T. Shishido, A. Shoda, D. H. Shoemaker, D. M. Shoemaker, S. ShyamSundar, M. Sieniawska, D. Sigg, L. Silenzi, L. P. Singer, D. Singh, M. K. Singh, N. Singh, A. Singha, A. M. Sintes, V. Sipala, V. Skliris, B. J. J. Slagmolen, T. J. Slaven-Blair, J. Smetana, J. R. Smith, L. Smith, R. J. E. Smith, J. Soldateschi, S. N. Somala, K. Somiya, I. Song, K. Soni, V. Sordini, F. Sorrentino, N. Sorrentino, R. Soulard, T. Souradeep, E. Sowell, V. Spagnuolo, A. P. Spencer, M. Spera, P. Spinicelli, A. K. Srivastava, V. Srivastava, K. Staats, C. Stachie, F. Stachurski, D. A. Steer, J. Steinlechner, S. Steinlechner, N. Stergioulas, D. J. Stops, M. Stover, K. A. Strain, L. C. Strang, G. Stratta, M. D. Strong, A. Strunk, R. Sturani, A. L. Stuver, M. Suchenek, S. Sudhagar, V. Sudhir, R. Sugimoto, H. G. Suh, A. G. Sullivan, T. Z. Summerscales, L. Sun, S. Sunil, A. Sur, J. Suresh, P. J. Sutton, Takamasa Suzuki, Takanori Suzuki, Toshikazu Suzuki, B. L. Swinkels, M. J. Szczepańczyk, P. Szewczyk, M. Tacca, H. Tagoshi, S. C. Tait, H. Takahashi, R. Takahashi, S. Takano, H. Takeda, M. Takeda, C. J. Talbot, C. Talbot, K. Tanaka, Taiki Tanaka, Takahiro Tanaka, A. J. Tanasijczuk, S. Tanioka, D. B. Tanner, D. Tao, L. Tao, R. D. Tapia, E. N. Tapia San Martín, C. Taranto, A. Taruya, J. D. Tasson, R. Tenorio, J. E. S. Terhune, L. Terkowski, M. P. Thirugnanasambandam, M. Thomas, P. Thomas, E. E. Thompson, J. E. Thompson, S. R. Thondapu, K. A. Thorne, E. Thrane, Shubhanshu Tiwari, Srishti Tiwari, V. Tiwari, A. M. Toivonen, A. E. Tolley, T. Tomaru, T. Tomura, M. Tonelli, Z. Tornasi, A. Torres-Forné, C. I. Torrie, I. Tosta e Melo, D. Töyrä, A. Trapananti, F. Travasso, G. Traylor, M. Trevor, M. C. Tringali, A. Tripathee, L. Troiano, A. Trovato, L. Trozzo, R. J. Trudeau, D. Tsai, K. W. Tsang, T. Tsang, J-S. Tsao, M. Tse, R. Tso, S. Tsuchida, L. Tsukada, D. Tsuna, T. Tsutsui, K. Turbang, M. Turconi, D. Tuyenbayev, A. S. Ubhi, N. Uchikata, T. Uchiyama, R. P. Udall, A. Ueda, T. Uehara, K. Ueno, G. Ueshima, C. S. Unnikrishnan, A. L. Urban, T. Ushiba, A. Utina, G. Vajente, A. Vajpeyi, G. Valdes, M. Valentini, V. Valsan, N. van Bakel, M. van Beuzekom, M. van Dael, J. F. J. van den Brand, C. Van Den Broeck, D. C. Vander-Hyde, H. van Haevermaet, J. V. van Heijningen, M. H. P. M. van Putten, N. van Remortel, M. Vardaro, A. F. Vargas, V. Varma, M. Vasúth, A. Vecchio, G. Vedovato, J. Veitch, P. J. Veitch, J. Venneberg, G. Venugopalan, D. Verkindt, P. Verma, Y. Verma, S. M. Vermeulen, D. Veske, F. Vetrano, A. Viceré, S. Vidyant, A. D. Viets, A. Vijaykumar, V. Villa-Ortega, J.-Y. Vinet, A. Virtuoso, S. Vitale, H. Vocca, E. R. G. von Reis, J. S. A. von Wrangel, C. Vorvick, S. P. Vyatchanin, L. E. Wade, M. Wade, K. J. Wagner, R. C. Walet, M. Walker, G. S. Wallace, L. Wallace, J. Wang, J. Z. Wang, W. H. Wang, R. L. Ward, J. Warner, M. Was, T. Washimi, N. Y. Washington, J. Watchi, B. Weaver, C. R. Weaving, S. A. Webster, M. Weinert, A. J. Weinstein, R. Weiss, C. M. Weller, R. A. Weller, F. Wellmann, L. Wen, P. Weßels, K. Wette, J. T. Whelan, D. D. White, B. F. Whiting, C. Whittle, D. Wilken, D. Williams, M. J. Williams, A. R. Williamson, J. L. Willis, B. Willke, D. J. Wilson, C. C. Wipf, T. Wlodarczyk, G. Woan, J. Woehler, J. K. Wofford, D. Wong, I. C. F. Wong, M. Wright, C. Wu, D. S. Wu, H. Wu, D. M. Wysocki, L. Xiao, T. Yamada, H. Yamamoto, K. Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, K. Z. Yang, L. Yang, Y.-C. Yang, Y. Yang, Yang Yang, M. J. Yap, D. W. Yeeles, S.-W. Yeh, A. B. Yelikar, M. Ying, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, R. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

    Physical Review D   105 ( 10 )   2022.05( ISSN:2470-0010 ( eISSN:2470-0029

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    This paper describes the first all-sky search for long-duration, quasimonochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20 to 610 Hz, over a small frequency derivative range around zero, and use multiple frequency resolutions to be robust towards possible signal frequency wanderings. Outliers from this search are followed up using two different methods, one more suitable for nearly monochromatic signals, and the other more robust towards frequency fluctuations. We do not find any evidence for such signals and set upper limits on the signal strain amplitude, the most stringent being ≈10-25 at around 130 Hz. We interpret these upper limits as both an "exclusion region"in the boson mass/black hole mass plane and the maximum detectable distance for a given boson mass, based on an assumption of the age of the black hole/boson cloud system.

    DOI: 10.1103/physrevd.105.102001

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.105.102001/fulltext

  • The Current Status and Future Prospects of KAGRA, the Large-Scale Cryogenic Gravitational Wave Telescope Built in the Kamioka Underground

    Homare Abe, Tomotada Akutsu, Masaki Ando, Akito Araya, Naoki Aritomi, Hideki Asada, Yoichi Aso, Sangwook Bae, Rishabh Bajpai, Kipp Cannon, Zhoujian Cao, Eleonora Capocasa, Man Chan, Dan Chen, Yi-Ru Chen, Marc Eisenmann, Raffaele Flaminio, Heather Fong, Yuta Fujikawa, Yuya Fujimoto, I. Hadiputrawan, Sadakazu Haino, Wenbiao Han, Kazuhiro Hayama, Yoshiaki Himemoto, Naoatsu Hirata, Chiaki Hirose, Tsung-Chieh Ho, Bin-Hua Hsieh, He-Feng Hsieh, Chia-Hsuan Hsiung, Hsiang-Yu Huang, Panwei Huang, Yao-Chin Huang, Yun-Jing Huang, David Hui, Kohei Inayoshi, Yuki Inoue, Yousuke Itoh, Pil-Jong Jung, Takaaki Kajita, Masahiro Kamiizumi, Nobuyuki Kanda, Takashi Kato, Chunglee Kim, Jaewan Kim, Young-Min Kim, Yuichiro Kobayashi, Kazunori Kohri, Keiko Kokeyama, Albert Kong, Naoki Koyama, Chihiro Kozakai, Jun’ya Kume, Sachiko Kuroyanagi, Kyujin Kwak, Eunsub Lee, Hyung Lee, Ray-Kuang Lee, Matteo Leonardi, Kwan-Lok Li, Pengbo Li, Lupin Lin, Chun-Yu Lin, En-Tzu Lin, Hong-Lin Lin, Guo-Chin Liu, Ling-Wei Luo, Miftahul Ma’arif, Yuta Michimura, Norikatsu Mio, Osamu Miyakawa, Kouseki Miyo, Shinji Miyoki, Nozomi Morisue, Kouji Nakamura, Hiroyuki Nakano, Masayuki Nakano, Tatsuya Narikawa, Lan Quynh, Takumi Nishimoto, Atsushi Nishizawa, Yoshihisa Obayashi, Kwangmin Oh, Masatake Ohashi, Tomoya Ohashi, Masashi Ohkawa, Yoshihiro Okutani, Ken-ichi Oohara, Shoichi Oshino, Kuo-Chuan Pan, Alessandro Parisi, June Park, Fabián Arellano, Surojit Saha, Kazuki Sakai, Takahiro Sawada, Yuichiro Sekiguchi, Lijing Shao, Yutaka Shikano, Hirotaka Shimizu, Katsuhiko Shimode, Hisaaki Shinkai, Ayaka Shoda, Kentaro Somiya, Inhyeok Song, Ryosuke Sugimoto, Jishnu Suresh, Takamasa Suzuki, Takanori Suzuki, Toshikazu Suzuki, Hideyuki Tagoshi, Hirotaka Takahashi, Ryutaro Takahashi, Hiroki Takeda, Mei Takeda, Atsushi Taruya, Takayuki Tomaru, Tomonobu Tomura, Lucia Trozzo, Terrence Tsang, Satoshi Tsuchida, Takuya Tsutsui, Darkhan Tuyenbayev, Nami Uchikata, Takashi Uchiyama, Tomoyuki Uehara, Koh Ueno, Takafumi Ushiba, Maurice Putten, Tatsuki Washimi, Chien-Ming Wu, Hsun-Chung Wu, Tomohiro Yamada, Kazuhiro Yamamoto, Takahiro Yamamoto, Ryo Yamazaki, Shu-Wei Yeh, Jun’ichi Yokoyama, Takaaki Yokozawa, Hirotaka Yuzurihara, Simon Zeidler, Yuhang Zhao

    Galaxies   10 ( 3 )   63 - 63   2022.04( eISSN:2075-4434

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    KAGRA is a gravitational-wave (GW) detector constructed in Japan with two unique key features: It was constructed underground, and the test-mass mirrors are cooled to cryogenic temperatures. These features are not included in other kilometer-scale detectors but will be adopted in future detectors such as the Einstein Telescope. KAGRA performed its first joint observation run with GEO600 in 2020. In this observation, the sensitivity of KAGRA to GWs was inferior to that of other kilometer-scale detectors such as LIGO and Virgo. However, further upgrades to the detector are ongoing to reach the sensitivity for detecting GWs in the next observation run, which is scheduled for 2022. In this article, the current situation, sensitivity, and future perspectives are reviewed.

    DOI: 10.3390/galaxies10030063

  • Relation between nutrition therapy in the acute phase and outcomes of ventilated patients with COVID-19 infection: A multicenter prospective observational study

    Nakamura K.

    American Journal of Clinical Nutrition   115 ( 4 )   1115 - 1122   2022.04( ISSN:00029165

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1093/ajcn/nqac014

  • Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b

    Abbott R.

    Astrophysical Journal   928 ( 2 )   2022.04( ISSN:0004637X

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/ac532b

  • Constraints on dark photon dark matter using data from LIGO’s and Virgo’s third observing run

    R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, C. Adams, N. Adhikari, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, S. Albanesi, A. Allocca, P. A. Altin, A. Amato, C. Anand, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, T. Andrade, N. Andres, T. Andrić, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, S. Appert, Koji Arai, Koya Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, S. M. Aronson, K. G. Arun, H. Asada, Y. Asali, G. Ashton, Y. Aso, M. Assiduo, S. M. Aston, P. Astone, F. Aubin, C. Austin, S. Babak, F. Badaracco, M. K. M. Bader, C. Badger, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, L. Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger, I. Belahcene, V. Benedetto, D. Beniwal, T. F. Bennett, J. D. Bentley, M. BenYaala, F. Bergamin, B. K. Berger, S. Bernuzzi, D. Bersanetti, A. Bertolini, J. Betzwieser, D. Beveridge, R. Bhandare, U. Bhardwaj, D. Bhattacharjee, S. Bhaumik, I. A. Bilenko, G. Billingsley, S. Bini, R. Birney, O. Birnholtz, S. Biscans, M. Bischi, S. Biscoveanu, A. Bisht, B. Biswas, M. Bitossi, M.-A. Bizouard, J. K. Blackburn, C. D. Blair, D. G. Blair, R. M. Blair, F. Bobba, N. Bode, M. Boer, G. Bogaert, M. Boldrini, L. D. Bonavena, F. Bondu, E. Bonilla, R. Bonnand, P. Booker, B. A. Boom, R. Bork, V. Boschi, N. Bose, S. Bose, V. Bossilkov, V. Boudart, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. R. Brady, A. Bramley, A. Branch, M. Branchesi, J. E. Brau, M. Breschi, T. Briant, J. H. Briggs, A. Brillet, M. Brinkmann, P. Brockill, A. F. Brooks, J. Brooks, D. D. Brown, S. Brunett, G. Bruno, R. Bruntz, J. Bryant, T. Bulik, H. J. Bulten, A. Buonanno, R. Buscicchio, D. Buskulic, C. Buy, R. L. Byer, L. Cadonati, G. Cagnoli, C. Cahillane, J. Calderón Bustillo, J. D. Callaghan, T. A. Callister, E. Calloni, J. Cameron, J. B. Camp, M. Canepa, S. Canevarolo, M. Cannavacciuolo, K. C. Cannon, H. Cao, Z. Cao, E. Capocasa, E. Capote, G. Carapella, F. Carbognani, J. B. Carlin, M. F. Carney, M. Carpinelli, G. Carrillo, G. Carullo, T. L. Carver, J. Casanueva Diaz, C. Casentini, G. Castaldi, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, M. Ceasar, G. Cella, P. Cerdá-Durán, E. Cesarini, W. Chaibi, K. Chakravarti, S. Chalathadka Subrahmanya, E. Champion, C.-H. Chan, C. Chan, C. L. Chan, K. Chan, M. Chan, K. Chandra, P. Chanial, S. Chao, P. Charlton, E. A. Chase, E. Chassande-Mottin, C. Chatterjee, Debarati Chatterjee, Deep Chatterjee, M. Chaturvedi, S. Chaty, C. Chen, H. Y. Chen, J. Chen, K. Chen, X. Chen, Y.-B. Chen, Y.-R. Chen, Z. Chen, H. Cheng, C. K. Cheong, H. Y. Cheung, H. Y. Chia, F. Chiadini, C-Y. Chiang, G. Chiarini, R. Chierici, A. Chincarini, M. L. Chiofalo, A. Chiummo, G. Cho, H. S. Cho, R. K. Choudhary, S. Choudhary, N. Christensen, H. Chu, Q. Chu, Y-K. Chu, S. Chua, K. W. Chung, G. Ciani, P. Ciecielag, M. Cieślar, M. Cifaldi, A. A. Ciobanu, R. Ciolfi, F. Cipriano, A. Cirone, F. Clara, E. N. Clark, J. A. Clark, L. Clarke, P. Clearwater, S. Clesse, F. Cleva, E. Coccia, E. Codazzo, P.-F. Cohadon, D. E. Cohen, L. Cohen, M. Colleoni, C. G. Collette, A. Colombo, M. Colpi, C. M. Compton, M. Constancio, L. Conti, S. J. Cooper, P. Corban, T. R. Corbitt, I. Cordero-Carrión, S. Corezzi, K. R. Corley, N. Cornish, D. Corre, A. Corsi, S. Cortese, C. A. Costa, R. Cotesta, M. W. Coughlin, J.-P. Coulon, S. T. Countryman, B. Cousins, P. Couvares, D. M. Coward, M. J. Cowart, D. C. Coyne, R. Coyne, J. D. E. Creighton, T. D. Creighton, A. W. Criswell, M. Croquette, S. G. Crowder, J. R. Cudell, T. J. Cullen, A. Cumming, R. Cummings, L. Cunningham, E. Cuoco, M. Curyło, P. Dabadie, T. Dal Canton, S. Dall’Osso, G. Dálya, A. Dana, L. M. DaneshgaranBajastani, B. D’Angelo, S. Danilishin, S. D’Antonio, K. Danzmann, C. Darsow-Fromm, A. Dasgupta, L. E. H. Datrier, S. Datta, V. Dattilo, I. Dave, M. Davier, G. S. Davies, D. Davis, M. C. Davis, E. J. Daw, R. Dean, D. DeBra, M. Deenadayalan, J. Degallaix, M. De Laurentis, S. Deléglise, V. Del Favero, F. De Lillo, N. De Lillo, W. Del Pozzo, L. M. DeMarchi, F. De Matteis, V. D’Emilio, N. Demos, T. Dent, A. Depasse, R. De Pietri, R. De Rosa, C. De Rossi, R. DeSalvo, R. De Simone, S. Dhurandhar, M. C. Díaz, M. Diaz-Ortiz, N. A. Didio, T. Dietrich, L. Di Fiore, C. Di Fronzo, C. Di Giorgio, F. Di Giovanni, M. Di Giovanni, T. Di Girolamo, A. Di Lieto, B. Ding, S. Di Pace, I. Di Palma, F. Di Renzo, A. K. Divakarla, A. Dmitriev, Z. Doctor, L. D’Onofrio, F. Donovan, K. L. Dooley, S. Doravari, I. Dorrington, M. Drago, J. C. Driggers, Y. Drori, J.-G. Ducoin, P. Dupej, O. 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    Physical Review D   105 ( 6 )   2022.03( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    We present a search for dark photon dark matter that could couple to gravitational-wave interferometers using data from Advanced LIGO and Virgo's third observing run. To perform this analysis, we use two methods, one based on cross-correlation of the strain channels in the two nearly aligned LIGO detectors, and one that looks for excess power in the strain channels of the LIGO and Virgo detectors. The excess power method optimizes the Fourier transform coherence time as a function of frequency, to account for the expected signal width due to Doppler modulations. We do not find any evidence of dark photon dark matter with a mass between mA∼10-14-10-11 eV/c2, which corresponds to frequencies between 10-2000 Hz, and therefore provide upper limits on the square of the minimum coupling of dark photons to baryons, i.e., U(1)B dark matter. For the cross-correlation method, the best median constraint on the squared coupling is ∼1.31×10-47 at mA∼4.2×10-13 eV/c2; for the other analysis, the best constraint is ∼2.4×10-47 at mA∼5.7×10-13 eV/c2. These limits improve upon those obtained in direct dark matter detection experiments by a factor of ∼100 for mA∼[2-4]×10-13 eV/c2, and are, in absolute terms, the most stringent constraint so far in a large mass range mA∼2×10-13-8×10-12 eV/c2.

    DOI: 10.1103/physrevd.105.063030

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.105.063030/fulltext

  • Search for intermediate-mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo

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Yamamoto, K. Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, L. Yang, Y. Yang, Yang Yang, Z. Yang, M. J. Yap, D. W. Yeeles, A. B. Yelikar, M. Ying, K. Yokogawa, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, H. Yu, H. Yuzurihara, A. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Y. Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

    Astronomy & Astrophysics   659   A84 - A84   2022.03( ISSN:0004-6361 ( eISSN:1432-0746

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    Publishing type:Research paper (scientific journal)  

    Intermediate-mass black holes (IMBHs) span the approximate mass range 100−10<sup>5</sup> M<sub>⊙</sub>, between black holes (BHs) that formed by stellar collapse and the supermassive BHs at the centers of galaxies. Mergers of IMBH binaries are the most energetic gravitational-wave sources accessible by the terrestrial detector network. Searches of the first two observing runs of Advanced LIGO and Advanced Virgo did not yield any significant IMBH binary signals. In the third observing run (O3), the increased network sensitivity enabled the detection of GW190521, a signal consistent with a binary merger of mass ∼150 M<sub>⊙</sub> providing direct evidence of IMBH formation. Here, we report on a dedicated search of O3 data for further IMBH binary mergers, combining both modeled (matched filter) and model-independent search methods. We find some marginal candidates, but none are sufficiently significant to indicate detection of further IMBH mergers. We quantify the sensitivity of the individual search methods and of the combined search using a suite of IMBH binary signals obtained via numerical relativity, including the effects of spins misaligned with the binary orbital axis, and present the resulting upper limits on astrophysical merger rates. Our most stringent limit is for equal mass and aligned spin BH binary of total mass 200 M<sub>⊙</sub> and effective aligned spin 0.8 at 0.056 Gpc<sup>−3</sup> yr<sup>−1</sup> (90% confidence), a factor of 3.5 more constraining than previous LIGO-Virgo limits. We also update the estimated rate of mergers similar to GW190521 to 0.08 Gpc<sup>−3</sup> yr<sup>−1</sup>.

    DOI: 10.1051/0004-6361/202141452

  • Search for continuous gravitational waves from 20 accreting millisecond x-ray pulsars in O3 LIGO data

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Xu, T. Yamada, H. Yamamoto, Kazuhiro Yamamoto, Kohei Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, L. Yang, Y. Yang, Yang Yang, Z. Yang, M. J. Yap, D. W. Yeeles, A. B. Yelikar, M. Ying, K. Yokogawa, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, M. E. Zucker, J. Zweizig, A. C. Albayati, D. Altamirano, P. Bult, D. Chakrabarty, M. Ng, P. S. Ray, A. Sanna, T. E. Strohmayer

    Physical Review D   105 ( 2 )   2022.01( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    Results are presented of searches for continuous gravitational waves from 20 accreting millisecond x-ray pulsars with accurately measured spin frequencies and orbital parameters, using data from the third observing run of the Advanced LIGO and Advanced Virgo detectors. The search algorithm uses a hidden Markov model, where the transition probabilities allow the frequency to wander according to an unbiased random walk, while the J-statistic maximum-likelihood matched filter tracks the binary orbital phase. Three narrow subbands are searched for each target, centered on harmonics of the measured spin frequency. The search yields 16 candidates, consistent with a false alarm probability of 30% per subband and target searched. These candidates, along with one candidate from an additional target-of-opportunity search done for SAX J1808.4-3658, which was in outburst during one month of the observing run, cannot be confidently associated with a known noise source. Additional follow-up does not provide convincing evidence that any are a true astrophysical signal. When all candidates are assumed nonastrophysical, upper limits are set on the maximum wave strain detectable at 95% confidence, h095%. The strictest constraint is h095%=4.7×10-26 from IGR J17062-6143. Constraints on the detectable wave strain from each target lead to constraints on neutron star ellipticity and r-mode amplitude, the strictest of which are ϵ95%=3.1×10-7 and α95%=1.8×10-5 respectively. This analysis is the most comprehensive and sensitive search of continuous gravitational waves from accreting millisecond x-ray pulsars to date.

    DOI: 10.1103/physrevd.105.022002

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.105.022002/fulltext

  • All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

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Woan, J. Woehler, J. K. Wofford, I. C. F. Wong, C. Wu, D. S. Wu, H. Wu, S. Wu, D. M. Wysocki, L. Xiao, W-R. Xu, T. Yamada, H. Yamamoto, Kazuhiro Yamamoto, Kohei Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, L. Yang, Y. Yang, Yang Yang, Z. Yang, M. J. Yap, D. W. Yeeles, A. B. Yelikar, M. Ying, K. Yokogawa, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

    Physical Review D   104 ( 12 )   2021.12( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24-4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization, or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as X10-10 Moc2 in gravitational waves at -70 Hz from a distance of 10 kpc, with 50% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.

    DOI: 10.1103/physrevd.104.122004

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.104.122004/fulltext

  • All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

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    PHYSICAL REVIEW D   104 ( 10 )   2021.11( ISSN:2470-0010

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.104.102001

  • All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

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Yamamoto, Kazuhiro Yamamoto, Kohei Yamamoto, T. Yamamoto, K. Yamashita, R. Yamazaki, F. W. Yang, L. Yang, Y. Yang, Yang Yang, Z. Yang, M. J. Yap, D. W. Yeeles, A. B. Yelikar, M. Ying, K. Yokogawa, J. Yokoyama, T. Yokozawa, J. Yoo, T. Yoshioka, Hang Yu, Haocun Yu, H. Yuzurihara, A. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, M. Zhan, H. Zhang, J. Zhang, L. Zhang, T. Zhang, Y. Zhang, C. Zhao, G. Zhao, Y. Zhao, Yue Zhao, R. Zhou, Z. Zhou, X. J. Zhu, Z.-H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

    Physical Review D   104 ( 10 )   2021.11( ISSN:2470-0010 ( eISSN:2470-0029

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    Publishing type:Research paper (scientific journal)  

    After the detection of gravitational waves from compact binary coalescences, the search for transient gravitational-wave signals with less well-defined waveforms for which matched filtering is not well suited is one of the frontiers for gravitational-wave astronomy. Broadly classified into "short" less than or similar to 1 s and "long" greater than or similar to 1 s duration signals, these signals are expected from a variety of astrophysical processes, including non-axisymmetric deformations in magnetars or eccentric binary black hole coalescences. In this work, we present a search for long-duration gravitational-wave transients from Advanced LIGO and Advanced Virgo's third observing run from April 2019 to March 2020. For this search, we use minimal assumptions for the sky location, event time, waveform morphology, and duration of the source. The search covers the range of 2-500 s in duration and a frequency band of 24-2048 Hz. We find no significant triggers within this parameter space; we report sensitivity limits on the signal strength of gravitational waves characterized by the root-sum-square amplitude h(rss) as a function of waveform morphology. These hrss limits improve upon the results from the second observing run by an average factor of 1.8.

    DOI: 10.1103/physrevd.104.102001

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.104.102001/fulltext

  • Constraints from LIGO O3 Data on Gravitational-wave Emission Due to R-modes in the Glitching Pulsar PSR J0537–6910

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Zhao, Yue Zhao, Yuhang Zhao, Z. Zhou, X. J. Zhu, Z.-H. Zhu, A. Zicoschi, M. E. Zucker, J. Zweizig, D. Antonopoulou, Z. Arzoumanian, T. Enoto, C. M. Espinoza, S. Guillot

    The Astrophysical Journal   922 ( 1 )   71 - 71   2021.11( ISSN:0004-637X ( eISSN:1538-4357

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    Publishing type:Research paper (scientific journal)  

    Abstract

    We present a search for continuous gravitational-wave emission due to r-modes in the pulsar PSR J0537–6910 using data from the LIGO–Virgo Collaboration observing run O3. PSR J0537–6910 is a young energetic X-ray pulsar and is the most frequent glitcher known. The inter-glitch braking index of the pulsar suggests that gravitational-wave emission due to r-mode oscillations may play an important role in the spin evolution of this pulsar. Theoretical models confirm this possibility and predict emission at a level that can be probed by ground-based detectors. In order to explore this scenario, we search for r-mode emission in the epochs between glitches by using a contemporaneous timing ephemeris obtained from NICER data. We do not detect any signals in the theoretically expected band of 86–97 Hz, and report upper limits on the amplitude of the gravitational waves. Our results improve on previous amplitude upper limits from r-modes in J0537-6910 by a factor of up to 3 and place stringent constraints on theoretical models for r-mode-driven spin-down in PSR J0537–6910, especially for higher frequencies at which our results reach below the spin-down limit defined by energy conservation.

    DOI: 10.3847/1538-4357/ac0d52

    Other URL: https://iopscience.iop.org/article/10.3847/1538-4357/ac0d52/pdf

  • Searches for Continuous Gravitational Waves from Young Supernova Remnants in the Early Third Observing Run of Advanced LIGO and Virgo

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Zhou, X. J. Zhu, Z.-H. Zhu, M. E. Zucker, J. Zweizig

    The Astrophysical Journal   921 ( 1 )   80 - 80   2021.11( ISSN:0004-637X ( eISSN:1538-4357

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    Publishing type:Research paper (scientific journal)  

    We present results of three wide-band directed searches for continuous gravitational waves from 15 young supernova remnants in the first half of the third Advanced LIGO and Virgo observing run. We use three search pipelines with distinct signal models and methods of identifying noise artifacts. Without ephemerides of these sources, the searches are conducted over a fRequency band spanning from 10 to 2 kHz. We find no evidence of continuous gravitational radiation from these sources. We set upper limits on the intrinsic signal strain at 95% confidence level in sample subbands, estimate the sensitivity in the full band, and derive the corresponding constraints on the fiducial neutron star ellipticity and r-mode amplitude. The best 95% confidence constraints placed on the signal strain are 7.7 × 10-26 and 7.8 × 10-26 near 200 Hz for the supernova remnants G39.2-0.3 and G65.7+1.2, respectively. The most stringent constraints on the ellipticity and r-mode amplitude reach ≲10-7 and ≲ 10-5, respectively, at frequencies above ∼400 Hz for the closest supernova remnant G266.2-1.2/Vela Jr.

    DOI: 10.3847/1538-4357/ac17ea

    Other URL: https://iopscience.iop.org/article/10.3847/1538-4357/ac17ea/pdf

  • Constraints from LIGO O3 Data on Gravitational-wave Emission Due to R-modes in the Glitching Pulsar PSR J0537-6910

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    ASTROPHYSICAL JOURNAL   922 ( 1 )   2021.11( ISSN:0004-637X

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/1538-4357/ac0d52

  • Searches for Continuous Gravitational Waves from Young Supernova Remnants in the Early Third Observing Run of Advanced LIGO and Virgo

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    PHYSICAL REVIEW D   104 ( 8 )   2021.10( ISSN:2470-0010

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.104.082004

  • Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

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    PHYSICAL REVIEW D   104 ( 2 )   2021.07( ISSN:2470-0010

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.104.022005

  • Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo's third observing run

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    ASTROPHYSICAL JOURNAL LETTERS   915 ( 1 )   2021.07( ISSN:2041-8205

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.3847/2041-8213/ac082e

  • Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run

    R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, K. M. Aleman, G. Allen, A. Allocca, P. A. Altin, A. Amato, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, S. Appert, Koya Arai, Koji Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, S. M. Aronson, H. Asada, Y. Asali, G. Ashton, Y. Aso, S. M. Aston, P. Astone, F. Aubin, P. Auclair, P. Aufmuth, K. Aultoneal, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, L. Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, M. Bals, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, R. S. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger, I. Belahcene

    Physical Review Letters   126 ( 24 )   2021.06( ISSN:0031-9007

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    We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks, and, for the first time, kink-kink collisions. A template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension Gμ as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models. Additionally, we develop and test a third model that interpolates between these two models. Our results improve upon the previous LIGO-Virgo constraints on Gμ by 1 to 2 orders of magnitude depending on the model that is tested. In particular, for the one-loop distribution model, we set the most competitive constraints to date: Gμ≲4×10-15. In the case of cosmic strings formed at the end of inflation in the context of grand unified theories, these results challenge simple inflationary models.

    DOI: 10.1103/PhysRevLett.126.241102

  • Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run

    R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, K. M. Aleman, G. Allen, A. Allocca, P. A. Altin, A. Amato, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, S. Appert, Koya Arai, Koji Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, S. M. Aronson, H. Asada, Y. Asali, G. Ashton, Y. Aso, S. M. Aston, P. Astone, F. Aubin, P. Auclair, P. Aufmuth, K. Aultoneal, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, L. Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, M. Bals, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, R. S. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger, I. Belahcene

    Physical Review Letters   126 ( 24 )   2021.06( ISSN:0031-9007 ( eISSN:1079-7114

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    Publishing type:Research paper (scientific journal)  

    We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks, and, for the first time, kink-kink collisions. A template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension Gμ as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models. Additionally, we develop and test a third model that interpolates between these two models. Our results improve upon the previous LIGO-Virgo constraints on Gμ by 1 to 2 orders of magnitude depending on the model that is tested. In particular, for the one-loop distribution model, we set the most competitive constraints to date: Gμ≲4×10-15. In the case of cosmic strings formed at the end of inflation in the context of grand unified theories, these results challenge simple inflationary models.

    DOI: 10.1103/PhysRevLett.126.241102

    PubMed

  • Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910

    R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, K. M. Aleman, G. Allen, A. Allocca, P. A. Altin, A. Amato, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, S. Appert, Koya Arai, Koji Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arene, N. Aritomi, N. Arnaud, S. M. Aronson, K. G. Arun, H. Asada, Y. Asali, G. Ashton, Y. Aso, S. M. Aston, P. Astone, F. Aubin, P. Aufmuth, K. Aultoneal, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, L. Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, M. Bals, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, R. S. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger, I. Belahcene

    Astrophysical Journal Letters   913 ( 2 )   2021.06( ISSN:2041-8205

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    We present a search for quasi-monochromatic gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using Neutron star Interior Composition Explorer (NICER) data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and exhibits fRequent and strong glitches. Analyses of its long-term and interglitch braking indices provide intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz rotation frequency also puts its possible gravitational-wave emission in the most sensitive band of the LIGO/Virgo detectors. Motivated by these considerations, we search for gravitational-wave emission at both once and twice the rotation frequency from PSR J0537-6910. We find no signal, however, and report upper limits. Assuming a rigidly rotating triaxial star, our constraints reach below the gravitational-wave spin-down limit for this star for the first time by more than a factor of 2 and limit gravitational waves from the l = m = 2 mode to account for less than 14% of the spin-down energy budget. The fiducial equatorial ellipticity is constrained to less than about 3 ×10-5, which is the third best constraint for any young pulsar.

    DOI: 10.3847/2041-8213/abffcd

  • Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910

    R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, K. M. Aleman, G. Allen, A. Allocca, P. A. Altin, A. Amato, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, S. Appert, Koya Arai, Koji Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arene, N. Aritomi, N. Arnaud, S. M. Aronson, K. G. Arun, H. Asada, Y. Asali, G. Ashton, Y. Aso, S. M. Aston, P. Astone, F. Aubin, P. Aufmuth, K. Aultoneal, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, L. Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, M. Bals, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, R. S. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger, I. Belahcene

    Astrophysical Journal Letters   913 ( 2 )   2021.06( ISSN:2041-8205 ( eISSN:2041-8213

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    Publishing type:Research paper (scientific journal)  

    We present a search for quasi-monochromatic gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using Neutron star Interior Composition Explorer (NICER) data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and exhibits fRequent and strong glitches. Analyses of its long-term and interglitch braking indices provide intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz rotation frequency also puts its possible gravitational-wave emission in the most sensitive band of the LIGO/Virgo detectors. Motivated by these considerations, we search for gravitational-wave emission at both once and twice the rotation frequency from PSR J0537-6910. We find no signal, however, and report upper limits. Assuming a rigidly rotating triaxial star, our constraints reach below the gravitational-wave spin-down limit for this star for the first time by more than a factor of 2 and limit gravitational waves from the l = m = 2 mode to account for less than 14% of the spin-down energy budget. The fiducial equatorial ellipticity is constrained to less than about 3 ×10-5, which is the third best constraint for any young pulsar.

    DOI: 10.3847/2041-8213/abffcd

  • Overview of KAGRA: Calibration, detector characterization, physical environmental monitors, and the geophysics interferometer

    Akutsu T.

    Progress of Theoretical and Experimental Physics   2021 ( 5 )   2021.05

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    DOI: 10.1093/ptep/ptab018

  • Current status of space gravitational wave antenna DECIGO and B-DECIGO

    Kawamura Seiji, Ando Masaki, Seto Naoki, Sato Shuichi, Musha Mitsuru, Kawano Isao, Yokoyama Jun'ichi, Tanaka Takahiro, Ioka Kunihito, Akutsu Tomotada, Takashima Takeshi, Agatsuma Kazuhiro, Araya Akito, Aritomi Naoki, Asada Hideki, Chiba Takeshi, Eguchi Satoshi, Enoki Motohiro, Fujimoto Masa-Katsu, Fujita Ryuichi, Futamase Toshifumi, Harada Tomohiro, Hayama Kazuhiro, Himemoto Yoshiaki, Hiramatsu Takashi, Hong Feng-Lei, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikari Satoshi, Ishihara Hideki, Ishikawa Tomohiro, Itoh Yousuke, Ito Takahiro, Iwaguchi Shoki, Izumi Kiwamu, Kanda Nobuyuki, Kanemura Shinya, Kawazoe Fumiko, Kobayashi Shiho, Kohri Kazunori, Kojima Yasufumi, Kokeyama Keiko, Kotake Kei, Kuroyanagi Sachiko, Maeda Kei-ichi, Matsushita Shuhei, Michimura Yuta, Morimoto Taigen, Mukohyama Shinji, Nagano Koji, Nagano Shigeo, Naito Takeo, Nakamura Kouji, Nakamura Takashi, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nakazawa Kazuhiro, Nishizawa Atsushi, Ohkawa Masashi, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Sakagami Masaaki, Sakai Shin-ichiro, Sato Takashi, Shibata Masaru, Shinkai Hisaaki, Shoda Ayaka, Somiya Kentaro, Sotani Hajime, Takahashi Ryutaro, Takahashi Hirotaka, Akiteru Takamori, Taniguchi Keisuke, Taruya Atsushi, Tsubono Kimio, Tsujikawa Shinji, Ueda Akitoshi, Ueda Ken-ichi, Watanabe Izumi, Yagi Kent, Yamada Rika, Yokoyama Shuichiro, Yoo Chul-Moon, Zhu Zong-Hong

    PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS   2021 ( 5 )   2021.05( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptab019

  • Overview of KAGRA: Calibration, detector characterization, physical environmental monitors, and the geophysics interferometer

    Akutsu T., Ando M., Arai K., Arai Y., Araki S., Araya A., Aritomi N., Asada H., Aso Y., Bae S., Baiotti L., Bajpai R., Barton M. A., Cannon K., Cao Z., Capocasa E., Chan M., Chen C., Chen K., Chen Y., Chiang C-Y, Chu H., Chu Y-K, Eguchi S., Enomoto Y., Flaminio R., Fujii Y., Fujikawa Y., Fukunaga M., Fukushima M., Gao D., Ge G., Ha S., Hagiwara A., Haino S., Han W-B, Hasegawa K., Hattori K., Hayakawa H., Hayama K., Himemoto Y., Hiranuma Y., Hirata N., Hirose E., Hong Z., Hsieh B., Huang G-Z, Huang H-Y, Huang P., Huang Y-C, Huang Y., Hui D. C. Y., Ide S., Ikenoue B., Imam S., Inayoshi K., Inoue Y., Ioka K., Ito K., Itoh Y., Izumi K., Jeon C., Jin H-B, Jung K., Jung P., Kaihotsu K., Kajita T., Kakizaki M., Kamiizumi M., Kanda N., Kang G., Kawaguchi K., Kawai N., Kawasaki T., Kim C., Kim J., Kim J. C., Kim S., Kim Y-M, Kimura N., Kita N., Kitazawa H., Kojima Y., Kokeyama K., Komori K., Kong A. K. H., Kotake K., Kozakai C., Kozu R., Kumar R., Kume J., Kuo C., Kuo H-S, Kuromiya Y., Kuroyanagi S., Kusayanagi K., Kwak K., Lee K., Lee H. W., Lee R., Leonardi M., Li K. L., Lin L. C-C, Lin F-K, Lin C-Y, Lin F-L, Lin H. L., Liu C., Luo L-W, Majorana E., Marchio M., Michimura Y., Mio N., Miyakawa O., Miyamoto A., Miyazaki Y., Miyo K., Miyoki S., Mori Y., Morisaki S., Moriwaki Y., Nagano K., Nagano S., Nakamura K., Nakano H., Nakano M., Nakashima R., Nakayama Y., Narikawa T., Naticchioni L., Negishi R., Quynh L. Nguyen, Ni W-T, Nishizawa A., Nozaki S., Obuchi Y., Ogaki W., Oh J. J., Oh K., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Ohta H., Okutani Y., Okutomi K., Oohara K., Ooi C., Oshino S., Otabe S., Pan K., Pang H., Parisi A., Park J., Arellano F. E. Pena, Pinto I, Sago N., Saito S., Saito Y., Sakai K., Sakai Y., Sakuno Y., Sato S., Sato T., Sawada T., Sekiguchi T., Sekiguchi Y., Shao L., Shibagaki S., Shimizu R., Shimoda T., Shimode K., Shinkai H., Shishido T., Shoda A., Somiya K., Son J., Sotani H., Sugimoto R., Suresh J., Suzuki T., Tagoshi H., Takahashi H., Takahashi R., Takamori A., Takano S., Takeda H., Takeda M., Tanaka H., Tanaka K., Tanaka T., Tanioka S., San Martin E. N. Tapia, Telada S., Tomaru T., Tomigami Y., Tomura T., Travasso F., Trozzo L., Tsang T., Tsao J-S, Tsubono K., Tsuchida S., Tsutsui T., Tsuzuki T., Tuyenbayev D., Uchikata N., Uchiyama T., Ueda A., Uehara T., Ueno K., Ueshima G., Uraguchi F., Ushiba T., van Putten M. H. P. M., Vocca H., Wang J., Washimi T., Wu C., Wu H., Wu S., Xu W-R, Yamada T., Yamamoto K., Yamamoto T., Yamashita K., Yamazaki R., Yang Y., Yokogawa K., Yokoyama J., Yokozawa T., Yoshioka T., Yuzurihara H., Zeidler S., Zhan M., Zhang H., Zhao Y., Zhu Z-H

    PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS   2021 ( 5 )   2021.05( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptab018

  • Gravitational Wave Physics and Astronomy in the nascent era

    Makoto Arimoto, Hideki Asada, Michael L Cherry, Michiko S Fujii, Yasushi Fukazawa, Akira Harada, Kazuhiro Hayama, Takashi Hosokawa, Kunihito Ioka, Yoichi Itoh, Nobuyuki Kanda, Koji S Kawabata, Kyohei Kawaguchi, Nobuyuki Kawai, Tsutomu Kobayashi, Kazunori Kohri, Yusuke Koshio, Kei Kotake, Jun Kumamoto, Masahiro N Machida, Hideo Matsufuru, Tatehiro Mihara, Masaki Mori, Tomoki Morokuma, Shinji Mukohyama, Hiroyuki Nakano, Tatsuya Narikawa, Hitoshi Negoro, Atsushi Nishizawa, Takayuki Ohgami, Kazuyuki Omukai, Takanori Sakamoto, Shigeyuki Sako, Mahito Sasada, Yuichiro Sekiguchi, Motoko Serino, Jiro Soda, Satoshi Sugita, Kohsuke Sumiyoshi, Hajime Susa, Teruaki Suyama, Hirotaka Takahashi, Kazuya Takahashi, Tomoya Takiwaki, Takahiro Tanaka, Masaomi Tanaka, Ataru Tanikawa, Nozomu Tominaga, Nami Uchikata, Yousuke Utsumi, Mark R Vagins, Kei Yamada, Michitoshi Yoshida

    Oxford University Press (OUP) Progress of Theoretical and Experimental Physics   2021.04

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    <title>Abstract</title>
    The detections of gravitational waves (GW) by LIGO/Virgo collaborations provide various possibilities to physics and astronomy. We are quite sure that GW observations will develop a lot both in precision and in number owing to the continuous works for the improvement of detectors, including the expectation to the newly joined detector, KAGRA, and the planned detector, LIGO-India. In this occasion, we review the fundamental outcomes and prospects of gravitational wave physics and astronomy. We survey the development focusing on representative sources of gravitational waves: binary black holes, binary neutron stars, and supernovae. We also summarize the role of gravitational wave observations as a probe of new physics.

    DOI: 10.1093/ptep/ptab042

  • Gravitational Wave Physics and Astronomy in the nascent era

    Makoto Arimoto, Hideki Asada, Michael L Cherry, Michiko S Fujii, Yasushi Fukazawa, Akira Harada, Kazuhiro Hayama, Takashi Hosokawa, Kunihito Ioka, Yoichi Itoh, Nobuyuki Kanda, Koji S Kawabata, Kyohei Kawaguchi, Nobuyuki Kawai, Tsutomu Kobayashi, Kazunori Kohri, Yusuke Koshio, Kei Kotake, Jun Kumamoto, Masahiro N Machida, Hideo Matsufuru, Tatehiro Mihara, Masaki Mori, Tomoki Morokuma, Shinji Mukohyama, Hiroyuki Nakano, Tatsuya Narikawa, Hitoshi Negoro, Atsushi Nishizawa, Takayuki Ohgami, Kazuyuki Omukai, Takanori Sakamoto, Shigeyuki Sako, Mahito Sasada, Yuichiro Sekiguchi, Motoko Serino, Jiro Soda, Satoshi Sugita, Kohsuke Sumiyoshi, Hajime Susa, Teruaki Suyama, Hirotaka Takahashi, Kazuya Takahashi, Tomoya Takiwaki, Takahiro Tanaka, Masaomi Tanaka, Ataru Tanikawa, Nozomu Tominaga, Nami Uchikata, Yousuke Utsumi, Mark R Vagins, Kei Yamada, Michitoshi Yoshida

    Progress of Theoretical and Experimental Physics   2021.04( eISSN:2050-3911

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    Publishing type:Research paper (scientific journal)  

    <title>Abstract</title>
    The detections of gravitational waves (GW) by LIGO/Virgo collaborations provide various possibilities to physics and astronomy. We are quite sure that GW observations will develop a lot both in precision and in number owing to the continuous works for the improvement of detectors, including the expectation to the newly joined detector, KAGRA, and the planned detector, LIGO-India. In this occasion, we review the fundamental outcomes and prospects of gravitational wave physics and astronomy. We survey the development focusing on representative sources of gravitational waves: binary black holes, binary neutron stars, and supernovae. We also summarize the role of gravitational wave observations as a probe of new physics.

    DOI: 10.1093/ptep/ptab042

  • Radiative Cooling of the Thermally Isolated System in KAGRA Gravitational Wave Telescope

    T. Akutsu, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya, N. Aritomi, Y. Aso, S. W. Bae, Y. B. Bae, L. Baiotti, R. Bajpai, M. A. Barton, K. Cannon, E. Capocasa, M. L. Chan, C. S. Chen, K. H. Chen, Y. R. Chen, H. Y. Chu, Y. K. Chu, S. Eguchi, Y. Enomoto, R. Flaminio, Y. Fujii, M. Fukunaga, M. Fukushima, G. G. Ge, A. Hagiwara, S. Haino, K. Hasegawa, H. Hayakawa, K. Hayama, Y. Himemoto, Y. Hiranuma, N. Hirata, E. Hirose, Z. Hong, B. H. Hsieh, G. Z. Huang, P. W. Huang, Y. J. Huang, B. Ikenoue, S. Imam, K. Inayoshi, Y. Inoue, K. Ioka, Y. Itoh, K. Izumi, K. Jung, P. Jung, T. Kajita, M. Kamiizumi, N. Kanda, G. W. Kang, K. Kawaguchi, N. Kawai, T. Kawasaki, C. Kim, J. Kim, W. Kim, Y. M. Kim, N. Kimura, N. Kita, H. Kitazawa, Y. Kojima, K. Kokeyama, K. Komori, A. K.H. Kong, K. Kotake, C. Kozakai, R. Kozu, R. Kumar, J. Kume, C. M. Kuo, H. S. Kuo, S. Kuroyanagi, K. Kusayanagi, K. Kwak, H. K. Lee, H. W. Lee, R. K. Lee, M. Leonardi, C. Y. Lin, F. L. Lin, L. C.C. Lin, G. C. Liu, L. W. Luo, M. Marchio, Y. Michimura, N. Mio, O. Miyakawa, A. Miyamoto, Y. Miyazaki, K. Miyo, S. Miyoki, S. Morisaki, Y. Moriwaki, K. Nagano, S. Nagano

    Journal of Physics: Conference Series   1857 ( 1 )   2021.04( ISSN:1742-6588

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    Radiative cooling of the thermally isolated system is investigated in KAGRA gravitational wave telescope. KAGRA is a laser interferometer-based detector and main mirrors constituting optical cavities are cool down to 20K to reduce noises caused by the thermal fluctuation. The mirror is suspended with the multi-stage pendulum to isolate any vibration. Therefore, this mirror suspension system has few heat links to reduce vibration injection. Thus, this system is mainly cooled down with thermal radiation. In order to understand the process of radiative cooling of the mirror, we analyzed cooling curve based on mass and specific heat. As a result, it was newly found that a cryogenic part called "cryogenic duct-shield"seems to have large contribution in the beginning of the mirror cooling. This finding will help to design new cooling system for the next generation cryogenic gravitational wave detector.

    DOI: 10.1088/1742-6596/1857/1/012002

  • Radiative Cooling of the Thermally Isolated System in KAGRA Gravitational Wave Telescope

    T. Akutsu, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya, N. Aritomi, Y. Aso, S. W. Bae, Y. B. Bae, L. Baiotti, R. Bajpai, M. A. Barton, K. Cannon, E. Capocasa, M. L. Chan, C. S. Chen, K. H. Chen, Y. R. Chen, H. Y. Chu, Y. K. Chu, S. Eguchi, Y. Enomoto, R. Flaminio, Y. Fujii, M. Fukunaga, M. Fukushima, G. G. Ge, A. Hagiwara, S. Haino, K. Hasegawa, H. Hayakawa, K. Hayama, Y. Himemoto, Y. Hiranuma, N. Hirata, E. Hirose, Z. Hong, B. H. Hsieh, G. Z. Huang, P. W. Huang, Y. J. Huang, B. Ikenoue, S. Imam, K. Inayoshi, Y. Inoue, K. Ioka, Y. Itoh, K. Izumi, K. Jung, P. Jung, T. Kajita, M. Kamiizumi, N. Kanda, G. W. Kang, K. Kawaguchi, N. Kawai, T. Kawasaki, C. Kim, J. Kim, W. Kim, Y. M. Kim, N. Kimura, N. Kita, H. Kitazawa, Y. Kojima, K. Kokeyama, K. Komori, A. K.H. Kong, K. Kotake, C. Kozakai, R. Kozu, R. Kumar, J. Kume, C. M. Kuo, H. S. Kuo, S. Kuroyanagi, K. Kusayanagi, K. Kwak, H. K. Lee, H. W. Lee, R. K. Lee, M. Leonardi, C. Y. Lin, F. L. Lin, L. C.C. Lin, G. C. Liu, L. W. Luo, M. Marchio, Y. Michimura, N. Mio, O. Miyakawa, A. Miyamoto, Y. Miyazaki, K. Miyo, S. Miyoki, S. Morisaki, Y. Moriwaki, K. Nagano, S. Nagano

    Journal of Physics: Conference Series   1857 ( 1 )   2021.04( ISSN:1742-6588 ( eISSN:1742-6596

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    Publishing type:Research paper (international conference proceedings)  

    Radiative cooling of the thermally isolated system is investigated in KAGRA gravitational wave telescope. KAGRA is a laser interferometer-based detector and main mirrors constituting optical cavities are cool down to 20K to reduce noises caused by the thermal fluctuation. The mirror is suspended with the multi-stage pendulum to isolate any vibration. Therefore, this mirror suspension system has few heat links to reduce vibration injection. Thus, this system is mainly cooled down with thermal radiation. In order to understand the process of radiative cooling of the mirror, we analyzed cooling curve based on mass and specific heat. As a result, it was newly found that a cryogenic part called "cryogenic duct-shield"seems to have large contribution in the beginning of the mirror cooling. This finding will help to design new cooling system for the next generation cryogenic gravitational wave detector.

    DOI: 10.1088/1742-6596/1857/1/012002

  • Vibration isolation systems for the beam splitter and signal recycling mirrors of the KAGRA gravitational wave detector

    T. Akutsu, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya, N. Aritomi, H. Asada, Y. Aso, S. Bae, Y. Bae, L. Baiotti, R. Bajpai, M. A. Barton, K. Cannon, Z. Cao, E. Capocasa, M. Chan, C. Chen, K. Chen, Y. Chen, C. Y. Chiang, H. Chu, Y. K. Chu, S. Eguchi, Y. Enomoto, R. Flaminio, Y. Fujii, Y. Fujikawa, M. Fukunaga, M. Fukushima, D. Gao, G. Ge, S. Ha, A. Hagiwara, S. Haino, W. B. Han, K. Hasegawa, R. Hatoya, K. Hattori, H. Hayakawa, K. Hayama, Y. Himemoto, Y. Hiranuma, N. Hirata, E. Hirose, Z. Hong, B. Hsieh, G. Z. Huang, H. Y. Huang, P. Huang, Y. C. Huang, Y. Huang, D. C.Y. Hui, S. Ide, B. Ikenoue, S. Imam, K. Inayoshi, Y. Inoue, K. Ioka, K. Ito, Y. Itoh, K. Izumi, C. Jeon, H. B. Jin, K. Jung, P. Jung, K. Kaihotsu, T. Kajita, M. Kakizaki, M. Kamiizumi, N. Kanda, G. Kang, K. Kawaguchi, N. Kawai, T. Kawasaki, C. Kim, J. Kim, J. C. Kim, W. S. Kim, Y. M. Kim, N. Kimura, N. Kita, H. Kitazawa, Y. Kojima, K. Kokeyama, K. Komori, A. K.H. Kong, K. Kotake, C. Kozakai, R. Kozu, R. Kumar, J. Kume, C. Kuo, H. S. Kuo, Y. Kuromiya, S. Kuroyanagi, K. Kusayanagi, K. Kwak, H. K. Lee

    Classical and Quantum Gravity   38 ( 6 )   2021.03( ISSN:0264-9381

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    Publishing type:Research paper (scientific journal)  

    KAGRA is an underground interferometric gravitational wave detector which is currently being commissioned. This detector relies on high-performance vibration-isolation systems to suspend its key optical components. These suspensions come in four different configurations, of which the type-B is used for the beam splitter and signal recycling mirrors. The type-B suspension comprises the payload, three geometric anti-spring filters for vertical isolation and one inverted pendulum for horizontal isolation. The payload comprises the optic, its marionette and their recoil masses, which hold local displacement sensors and coil magnet actuators used for damping the resonant modes of oscillation of the suspension itself. The beam splitter version has a modified lower section to accommodate a wider optical component. The payload is also equipped with an optical lever, used to monitor and control the position of the suspended optics from the ground. All four suspensions have now been installed in vacuum chambers. We describe the mechanical, electrical and control design, and the measured performance compared to requirements.

    DOI: 10.1088/1361-6382/abd922

  • Vibration isolation systems for the beam splitter and signal recycling mirrors of the KAGRA gravitational wave detector

    T. Akutsu, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya, N. Aritomi, H. Asada, Y. Aso, S. Bae, Y. Bae, L. Baiotti, R. Bajpai, M. A. Barton, K. Cannon, Z. Cao, E. Capocasa, M. Chan, C. Chen, K. Chen, Y. Chen, C. Y. Chiang, H. Chu, Y. K. Chu, S. Eguchi, Y. Enomoto, R. Flaminio, Y. Fujii, Y. Fujikawa, M. Fukunaga, M. Fukushima, D. Gao, G. Ge, S. Ha, A. Hagiwara, S. Haino, W. B. Han, K. Hasegawa, R. Hatoya, K. Hattori, H. Hayakawa, K. Hayama, Y. Himemoto, Y. Hiranuma, N. Hirata, E. Hirose, Z. Hong, B. Hsieh, G. Z. Huang, H. Y. Huang, P. Huang, Y. C. Huang, Y. Huang, D. C.Y. Hui, S. Ide, B. Ikenoue, S. Imam, K. Inayoshi, Y. Inoue, K. Ioka, K. Ito, Y. Itoh, K. Izumi, C. Jeon, H. B. Jin, K. Jung, P. Jung, K. Kaihotsu, T. Kajita, M. Kakizaki, M. Kamiizumi, N. Kanda, G. Kang, K. Kawaguchi, N. Kawai, T. Kawasaki, C. Kim, J. Kim, J. C. Kim, W. S. Kim, Y. M. Kim, N. Kimura, N. Kita, H. Kitazawa, Y. Kojima, K. Kokeyama, K. Komori, A. K.H. Kong, K. Kotake, C. Kozakai, R. Kozu, R. Kumar, J. Kume, C. Kuo, H. S. Kuo, Y. Kuromiya, S. Kuroyanagi, K. Kusayanagi, K. Kwak, H. K. Lee

    Classical and Quantum Gravity   38 ( 6 )   2021.03( ISSN:0264-9381 ( eISSN:1361-6382

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    Publishing type:Research paper (scientific journal)  

    KAGRA is an underground interferometric gravitational wave detector which is currently being commissioned. This detector relies on high-performance vibration-isolation systems to suspend its key optical components. These suspensions come in four different configurations, of which the type-B is used for the beam splitter and signal recycling mirrors. The type-B suspension comprises the payload, three geometric anti-spring filters for vertical isolation and one inverted pendulum for horizontal isolation. The payload comprises the optic, its marionette and their recoil masses, which hold local displacement sensors and coil magnet actuators used for damping the resonant modes of oscillation of the suspension itself. The beam splitter version has a modified lower section to accommodate a wider optical component. The payload is also equipped with an optical lever, used to monitor and control the position of the suspended optics from the ground. All four suspensions have now been installed in vacuum chambers. We describe the mechanical, electrical and control design, and the measured performance compared to requirements.

    DOI: 10.1088/1361-6382/abd922

  • Current status of space gravitational wave antenna DECIGO and B-DECIGO

    Seiji Kawamura, Masaki Ando, Naoki Seto, Shuichi Sato, Mitsuru Musha, Isao Kawano, Jun’ichi Yokoyama, Takahiro Tanaka, Kunihito Ioka, Tomotada Akutsu, Takeshi Takashima, Kazuhiro Agatsuma, Akito Araya, Naoki Aritomi, Hideki Asada, Takeshi Chiba, Satoshi Eguchi, Motohiro Enoki, Masa-Katsu Fujimoto, Ryuichi Fujita, Toshifumi Futamase, Tomohiro Harada, Kazuhiro Hayama, Yoshiaki Himemoto, Takashi Hiramatsu, Feng-Lei Hong, Mizuhiko Hosokawa, Kiyotomo Ichiki, Satoshi Ikari, Hideki Ishihara, Tomohiro Ishikawa, Yousuke Itoh, Takahiro Ito, Shoki Iwaguchi, Kiwamu Izumi, Nobuyuki Kanda, Shinya Kanemura, Fumiko Kawazoe, Shiho Kobayashi, Kazunori Kohri, Yasufumi Kojima, Keiko Kokeyama, Kei Kotake, Sachiko Kuroyanagi, Kei-ichi Maeda, Shuhei Matsushita, Yuta Michimura, Taigen Morimoto, Shinji Mukohyama, Koji Nagano, Shigeo Nagano, Takeo Naito, Kouji Nakamura, Takashi Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Kazuhiro Nakazawa, Atsushi Nishizawa, Masashi Ohkawa, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Masaaki Sakagami, Shin-ichiro Sakai, Takashi Sato, Masaru Shibata, Hisaaki Shinkai, Ayaka Shoda, Kentaro Somiya, Hajime Sotani, Ryutaro Takahashi, Hirotaka Takahashi, Takamori Akiteru, Keisuke Taniguchi, Atsushi Taruya, Kimio Tsubono, Shinji Tsujikawa, Akitoshi Ueda, Ken-ichi Ueda, Izumi Watanabe, Kent Yagi, Rika Yamada, Shuichiro Yokoyama, Chul-Moon Yoo, Zong-Hong Zhu

    Progress of Theoretical and Experimental Physics   2021 ( 5 )   2021.02( eISSN:20503911

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    <jats:title>Abstract</jats:title>
    <jats:p>The Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO) is a future Japanese space mission with a frequency band of 0.1 Hz to 10 Hz. DECIGO aims at the detection of primordial gravitational waves, which could have been produced during the inflationary period right after the birth of the Universe. There are many other scientific objectives of DECIGO, including the direct measurement of the acceleration of the expansion of the Universe, and reliable and accurate predictions of the timing and locations of neutron star/black hole binary coalescences. DECIGO consists of four clusters of observatories placed in heliocentric orbit. Each cluster consists of three spacecraft, which form three Fabry–Pérot Michelson interferometers with an arm length of 1000 km. Three DECIGO clusters will be placed far from each other, and the fourth will be placed in the same position as one of the other three to obtain correlation signals for the detection of primordial gravitational waves. We plan to launch B-DECIGO, which is a scientific pathfinder for DECIGO, before DECIGO in the 2030s to demonstrate the technologies required for DECIGO, as well as to obtain fruitful scientific results to further expand multi-messenger astronomy.</jats:p>

    DOI: 10.1093/ptep/ptab019

  • Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA Reviewed

    B. P. Abbott, R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, C. Adams, V. B. Adya, C. Affeldt, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, G. Allen, A. Allocca, M. A. Aloy, P. A. Altin, A. Amato, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, S. V. Angelova, S. Antier, S. Appert, K. Arai, Koya Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, K. G. Arun, S. Ascenzi, G. Ashton, Y. Aso, S. M. Aston, P. Astone, F. Aubin, P. Aufmuth, K. AultONeal, C. Austin, V. Avendano, A. Avila-Alvarez, S. Babak, P. Bacon, F. Badaracco, M. K. M. Bader, S. W. Bae, Y. B. Bae, L. Baiotti, R. Bajpai, P. T. Baker, F. Baldaccini, G. Ballardin, S. W. Ballmer, S. Banagiri, J. C. Barayoga, S. E. Barclay, B. C. Barish, D. Barker, K. Barkett, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, M. Bazzan, B. Bécsy, M. Bejger, I. Belahcene, A. S. Bell, D. Beniwal, B. K. Berger, G. Bergmann, S. Bernuzzi, J. J. Bero, C. P. L. Berry, D. Bersanetti, A. Bertolini, J. Betzwieser, R. Bhandare, J. Bidler, I. A. Bilenko, S. A. Bilgili, G. Billingsley, J. Birch, R. Birney, O. Birnholtz, S. Biscans, S. Biscoveanu, A. Bisht, M. Bitossi, M. A. Bizouard, J. K. Blackburn, C. D. Blair, D. G. Blair, R. M. Blair, S. Bloemen, N. Bode, M. Boer, Y. Boetzel, G. Bogaert, F. Bondu, E. Bonilla, R. Bonnand, P. Booker, B. A. Boom, C. D. Booth, R. Bork, V. Boschi, S. Bose, K. Bossie, V. Bossilkov, J. Bosveld, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. R. Brady, A. Bramley, M. Branchesi, J. E. Brau, T. Briant, J. H. Briggs, F. Brighenti, A. Brillet, M. Brinkmann, V. Brisson, P. Brockill, A. F. Brooks, D. A. Brown, D. D. Brown, S. Brunett, A. Buikema, T. Bulik, H. J. Bulten, A. Buonanno, D. Buskulic, C. Buy, R. L. Byer, M. Cabero, L. Cadonati, G. Cagnoli, C. Cahillane, J. Calderón Bustillo, T. A. Callister, E. Calloni, J. B. Camp, W. A. Campbell, M. Canepa, K. Cannon, K. C. Cannon, H. Cao, J. Cao, E. Capocasa, F. Carbognani, S. Caride, M. F. Carney, G. Carullo, J. Casanueva Diaz, C. Casentini, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, G. Cella, P. Cerdá-Durán, G. Cerretani, E. Cesarini, O. Chaibi, K. Chakravarti, S. J. Chamberlin, M. Chan, M. L. Chan, S. Chao, P. Charlton, E. A. Chase, E. Chassande-Mottin, D. Chatterjee, M. Chaturvedi, K. Chatziioannou, B. D. Cheeseboro, C. S. Chen, H. Y. Chen, K. H. Chen, X. Chen, Y. Chen, Y. R. Chen, H.-P. Cheng, C. K. Cheong, H. Y. Chia, A. Chincarini, A. Chiummo, G. Cho, H. S. Cho, M. Cho, N. Christensen, H. Y. Chu, Q. Chu, Y. K. Chu, S. Chua, K. W. Chung, S. Chung, G. Ciani, A. A. Ciobanu, R. Ciolfi, F. Cipriano, A. Cirone, F. Clara, J. A. Clark, P. Clearwater, F. Cleva, C. Cocchieri, E. Coccia, P.-F. Cohadon, D. Cohen, R. Colgan, M. Colleoni, C. G. Collette, C. Collins, L. R. Cominsky, M. Constancio, L. Conti, S. J. Cooper, P. Corban, T. R. Corbitt, I. Cordero-Carrión, K. R. Corley, N. Cornish, A. Corsi, S. Cortese, C. A. Costa, R. Cotesta, M. W. Coughlin, S. B. Coughlin, J.-P. Coulon, S. T. Countryman, P. Couvares, P. B. Covas, E. E. Cowan, D. M. Coward, M. J. Cowart, D. C. Coyne, R. Coyne, J. D. E. Creighton, T. D. Creighton, J. Cripe, M. Croquette, S. G. Crowder, T. J. Cullen, A. Cumming, L. Cunningham, E. Cuoco, T. Dal Canton, G. Dálya, S. L. Danilishin, S. D’Antonio, K. Danzmann, A. Dasgupta, C. F. Da Silva Costa, L. E. H. Datrier, V. Dattilo, I. Dave, M. Davier, D. Davis, E. J. Daw, D. DeBra, M. Deenadayalan, J. Degallaix, M. De Laurentis, S. Deléglise, W. Del Pozzo, L. M. DeMarchi, N. Demos, T. Dent, R. De Pietri, J. Derby, R. De Rosa, C. De Rossi, R. DeSalvo, O. de Varona, S. Dhurandhar, M. C. Díaz, T. Dietrich, L. Di Fiore, M. Di Giovanni, T. Di Girolamo, A. Di Lieto, B. Ding, S. Di Pace, I. Di Palma, F. Di Renzo, A. Dmitriev, Z. Doctor, K. Doi, F. Donovan, K. L. Dooley, S. Doravari, I. Dorrington, T. P. Downes, M. Drago, J. C. Driggers, Z. Du, J.-G. Ducoin, P. Dupej, S. E. Dwyer, P. J. Easter, T. B. Edo, M. C. Edwards, A. Effler, S. Eguchi, P. Ehrens, J. Eichholz, S. S. Eikenberry, M. Eisenmann, R. A. Eisenstein, Y. Enomoto, R. C. Essick, H. Estelles, D. Estevez, Z. B. Etienne, T. Etzel, M. Evans, T. M. Evans, V. Fafone, H. Fair, S. Fairhurst, X. Fan, S. Farinon, B. Farr, W. M. Farr, E. J. Fauchon-Jones, M. Favata, M. Fays, M. Fazio, C. Fee, J. Feicht, M. M. Fejer, F. Feng, A. Fernandez-Galiana, I. Ferrante, E. C. Ferreira, T. A. Ferreira, F. Ferrini, F. Fidecaro, I. Fiori, D. Fiorucci, M. Fishbach, R. P. Fisher, J. M. Fishner, M. Fitz-Axen, R. Flaminio, M. Fletcher, E. Flynn, H. Fong, J. A. Font, P. W. F. Forsyth, J.-D. Fournier, S. Frasca, F. Frasconi, Z. Frei, A. Freise, R. Frey, V. Frey, P. Fritschel, V. V. Frolov, Y. Fujii, M. Fukunaga, M. Fukushima, P. Fulda, M. Fyffe, H. A. Gabbard, B. U. Gadre, S. M. Gaebel, J. R. Gair, L. Gammaitoni, M. R. Ganija, S. G. Gaonkar, A. Garcia, C. García-Quirós, F. Garufi, B. Gateley, S. Gaudio, G. Gaur, V. Gayathri, G. G. Ge, G. Gemme, E. Genin, A. Gennai, D. George, J. George, L. Gergely, V. Germain, S. Ghonge, Abhirup Ghosh, Archisman Ghosh, S. Ghosh, B. Giacomazzo, J. A. Giaime, K. D. Giardina, A. Giazotto, K. Gill, G. Giordano, L. Glover, P. Godwin, E. Goetz, R. Goetz, B. Goncharov, G. González, J. M. Gonzalez Castro, A. Gopakumar, M. L. Gorodetsky, S. E. Gossan, M. Gosselin, R. Gouaty, A. Grado, C. Graef, M. Granata, A. Grant, S. Gras, P. Grassia, C. Gray, R. Gray, G. Greco, A. C. Green, R. Green, E. M. Gretarsson, P. Groot, H. Grote, S. Grunewald, P. Gruning, G. M. Guidi, H. K. Gulati, Y. Guo, A. Gupta, M. K. Gupta, E. K. Gustafson, R. Gustafson, L. Haegel, A. Hagiwara, S. Haino, O. Halim, B. R. Hall, E. D. Hall, E. Z. Hamilton, G. Hammond, M. Haney, M. M. Hanke, J. Hanks, C. Hanna, M. D. Hannam, O. A. Hannuksela, J. Hanson, T. Hardwick, K. Haris, J. Harms, G. M. Harry, I. W. Harry, K. Hasegawa, C.-J. Haster, K. Haughian, H. Hayakawa, K. Hayama, F. J. Hayes, J. Healy, A. Heidmann, M. C. Heintze, H. Heitmann, P. Hello, G. Hemming, M. Hendry, I. S. Heng, J. Hennig, A. W. Heptonstall, M. Heurs, S. Hild, Y. Himemoto, T. Hinderer, Y. Hiranuma, N. Hirata, E. Hirose, D. Hoak, S. Hochheim, D. Hofman, A. M. Holgado, N. A. Holland, K. Holt, D. E. Holz, Z. Hong, P. Hopkins, C. Horst, J. Hough, E. J. Howell, C. G. Hoy, A. Hreibi, B. H. Hsieh, G. Z. Huang, P. W. Huang, Y. J. Huang, E. A. Huerta, D. Huet, B. Hughey, M. Hulko, S. Husa, S. H. Huttner, T. Huynh-Dinh, B. Idzkowski, A. Iess, B. Ikenoue, S. Imam, K. Inayoshi, C. Ingram, Y. Inoue, R. Inta, G. Intini, K. Ioka, B. Irwin, H. N. Isa, J.-M. Isac, M. Isi, Y. Itoh, B. R. Iyer, K. Izumi, T. Jacqmin, S. J. Jadhav, K. Jani, N. N. Janthalur, P. Jaranowski, A. C. Jenkins, J. Jiang, D. S. Johnson, A. W. Jones, D. I. Jones, R. Jones, R. J. G. Jonker, L. Ju, K. Jung, P. Jung, J. Junker, T. Kajita, C. V. Kalaghatgi, V. Kalogera, B. Kamai, M. Kamiizumi, N. Kanda, S. Kandhasamy, G. W. Kang, J. B. Kanner, S. J. Kapadia, S. Karki, K. S. Karvinen, R. Kashyap, M. Kasprzack, S. Katsanevas, E. Katsavounidis, W. Katzman, S. Kaufer, K. Kawabe, K. Kawaguchi, N. Kawai, T. Kawasaki, N. V. Keerthana, F. Kéfélian, D. Keitel, R. Kennedy, J. S. Key, F. Y. Khalili, H. Khan, I. Khan, S. Khan, Z. Khan, E. A. Khazanov, M. Khursheed, N. Kijbunchoo, Chunglee Kim, C. Kim, J. C. Kim, J. Kim, K. Kim, W. Kim, W. S. Kim, Y.-M. Kim, C. Kimball, N. Kimura, E. J. King, P. J. King, M. Kinley-Hanlon, R. Kirchhoff, J. S. Kissel, N. Kita, H. Kitazawa, L. Kleybolte, J. H. Klika, S. Klimenko, T. D. Knowles, E. Knyazev, P. Koch, S. M. Koehlenbeck, G. Koekoek, Y. Kojima, K. Kokeyama, S. Koley, K. Komori, V. Kondrashov, A. K. H. Kong, A. Kontos, N. Koper, M. Korobko, W. Z. Korth, K. Kotake, I. Kowalska, D. B. Kozak, C. Kozakai, R. Kozu, V. Kringel, N. Krishnendu, A. Królak, G. Kuehn, A. Kumar, P. Kumar, Rahul Kumar, R. Kumar, S. Kumar, J. Kume, C. M. Kuo, H. S. Kuo, L. Kuo, S. Kuroyanagi, K. Kusayanagi, A. Kutynia, K. Kwak, S. Kwang, B. D. Lackey, K. H. Lai, T. L. Lam, M. Landry, B. B. Lane, R. N. Lang, J. Lange, B. Lantz, R. K. Lanza, A. Lartaux-Vollard, P. D. Lasky, M. Laxen, A. Lazzarini, C. Lazzaro, P. Leaci, S. Leavey, Y. K. Lecoeuche, C. H. Lee, H. K. Lee, H. M. Lee, H. W. Lee, J. Lee, K. Lee, R. K. Lee, J. Lehmann, A. Lenon, M. Leonardi, N. Leroy, N. Letendre, Y. Levin, J. Li, K. J. L. Li, T. G. F. Li, X. Li, C. Y. Lin, F. Lin, F. L. Lin, L. C. C. Lin, F. Linde, S. D. Linker, T. B. Littenberg, G. C. Liu, J. Liu, X. Liu, R. K. L. Lo, N. A. Lockerbie, L. T. London, A. Longo, M. Lorenzini, V. Loriette, M. Lormand, G. Losurdo, J. D. Lough, C. O. Lousto, G. Lovelace, M. E. Lower, H. Lück, D. Lumaca, A. P. Lundgren, L. W. Luo, R. Lynch, Y. Ma, R. Macas, S. Macfoy, M. MacInnis, D. M. Macleod, A. Macquet, F. Magaña-Sandoval, L. Magaña Zertuche, R. M. Magee, E. Majorana, I. Maksimovic, A. Malik, N. Man, V. Mandic, V. Mangano, G. L. Mansell, M. Manske, M. Mantovani, F. Marchesoni, M. Marchio, F. Marion, S. Márka, Z. Márka, C. Markakis, A. S. Markosyan, A. Markowitz, E. Maros, A. Marquina, S. Marsat, F. Martelli, I. W. Martin, R. M. Martin, D. V. Martynov, K. Mason, E. Massera, A. Masserot, T. J. Massinger, M. Masso-Reid, S. Mastrogiovanni, A. Matas, F. Matichard, L. Matone, N. Mavalvala, N. Mazumder, J. J. McCann, R. McCarthy, D. E. McClelland, S. McCormick, L. McCuller, S. C. McGuire, J. McIver, D. J. McManus, T. McRae, S. T. McWilliams, D. Meacher, G. D. Meadors, M. Mehmet, A. K. Mehta, J. Meidam, A. Melatos, G. Mendell, R. A. Mercer, L. Mereni, E. L. Merilh, M. Merzougui, S. Meshkov, C. Messenger, C. Messick, R. Metzdorff, P. M. Meyers, H. Miao, C. Michel, Y. Michimura, H. Middleton, E. E. Mikhailov, L. Milano, A. L. Miller, A. Miller, M. Millhouse, J. C. Mills, M. C. Milovich-Goff, O. Minazzoli, Y. Minenkov, N. Mio, A. Mishkin, C. Mishra, T. Mistry, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, A. Miyamoto, Y. Miyazaki, K. Miyo, S. Miyoki, G. Mo, D. Moffa, K. Mogushi, S. R. P. Mohapatra, M. Montani, C. J. Moore, D. Moraru, G. Moreno, S. Morisaki, Y. Moriwaki, B. Mours, C. M. Mow-Lowry, Arunava Mukherjee, D. Mukherjee, S. Mukherjee, N. Mukund, A. Mullavey, J. Munch, E. A. Muñiz, M. Muratore, P. G. Murray, K. Nagano, S. Nagano, A. Nagar, K. Nakamura, H. Nakano, M. Nakano, R. Nakashima, I. Nardecchia, T. Narikawa, L. Naticchioni, R. K. Nayak, R. Negishi, J. Neilson, G. Nelemans, T. J. N. Nelson, M. Nery, A. Neunzert, K. Y. Ng, S. Ng, P. Nguyen, W. T. Ni, D. Nichols, A. Nishizawa, S. Nissanke, F. Nocera, C. North, L. K. Nuttall, M. Obergaulinger, J. Oberling, B. D. O’Brien, Y. Obuchi, G. D. O’Dea, W. Ogaki, G. H. Ogin, J. J. Oh, S. H. Oh, M. Ohashi, N. Ohishi, M. Ohkawa, F. Ohme, H. Ohta, M. A. Okada, K. Okutomi, M. Oliver, K. Oohara, C. P. Ooi, P. Oppermann, Richard J. Oram, B. O’Reilly, R. G. Ormiston, L. F. Ortega, R. O’Shaughnessy, S. Oshino, S. Ossokine, D. J. Ottaway, H. Overmier, B. J. Owen, A. E. Pace, G. Pagano, M. A. Page, A. Pai, S. A. Pai, J. R. Palamos, O. Palashov, C. Palomba, A. Pal-Singh, Huang-Wei Pan, K. C. Pan, B. Pang, H. F. Pang, P. T. H. Pang, C. Pankow, F. Pannarale, B. C. Pant, F. Paoletti, A. Paoli, M. A. Papa, A. Parida, J. Park, W. Parker, D. Pascucci, A. Pasqualetti, R. Passaquieti, D. Passuello, M. Patil, B. Patricelli, B. L. Pearlstone, C. Pedersen, M. Pedraza, R. Pedurand, A. Pele, F. E. Peña Arellano, S. Penn, C. J. Perez, A. Perreca, H. P. Pfeiffer, M. Phelps, K. S. Phukon, O. J. Piccinni, M. Pichot, F. Piergiovanni, G. Pillant, L. Pinard, I. Pinto, M. Pirello, M. Pitkin, R. Poggiani, D. Y. T. Pong, S. Ponrathnam, P. Popolizio, E. K. Porter, J. Powell, A. K. Prajapati, J. Prasad, K. Prasai, R. Prasanna, G. Pratten, T. Prestegard, S. Privitera, G. A. Prodi, L. G. Prokhorov, O. Puncken, M. Punturo, P. Puppo, M. Pürrer, H. Qi, V. Quetschke, P. J. Quinonez, E. A. Quintero, R. Quitzow-James, F. J. Raab, H. Radkins, N. Radulescu, P. Raffai, S. Raja, C. Rajan, B. Rajbhandari, M. Rakhmanov, K. E. Ramirez, A. Ramos-Buades, Javed Rana, K. Rao, P. Rapagnani, V. Raymond, M. Razzano, J. Read, T. Regimbau, L. Rei, S. Reid, D. H. Reitze, W. Ren, F. Ricci, C. J. Richardson, J. W. Richardson, P. M. Ricker, K. Riles, M. Rizzo, N. A. Robertson, R. Robie, F. Robinet, A. Rocchi, L. Rolland, J. G. Rollins, V. J. Roma, M. Romanelli, R. Romano, C. L. Romel, J. H. Romie, K. Rose, D. Rosińska, S. G. Rosofsky, M. P. Ross, S. Rowan, A. Rüdiger, P. Ruggi, G. Rutins, K. Ryan, S. Sachdev, T. Sadecki, N. Sago, S. Saito, Y. Saito, K. Sakai, Y. Sakai, H. Sakamoto, M. Sakellariadou, Y. Sakuno, L. Salconi, M. Saleem, A. Samajdar, L. Sammut, E. J. Sanchez, L. E. Sanchez, N. Sanchis-Gual, V. Sandberg, J. R. Sanders, K. A. Santiago, N. Sarin, B. Sassolas, B. S. Sathyaprakash, S. Sato, T. Sato, O. Sauter, R. L. Savage, T. Sawada, P. Schale, M. Scheel, J. Scheuer, P. Schmidt, R. Schnabel, R. M. S. Schofield, A. Schönbeck, E. Schreiber, B. W. Schulte, B. F. Schutz, S. G. Schwalbe, J. Scott, S. M. Scott, E. Seidel, T. Sekiguchi, Y. Sekiguchi, D. Sellers, A. S. Sengupta, N. Sennett, D. Sentenac, V. Sequino, A. Sergeev, Y. Setyawati, D. A. Shaddock, T. Shaffer, M. S. Shahriar, M. B. Shaner, L. Shao, P. Sharma, P. Shawhan, H. Shen, S. Shibagaki, R. Shimizu, T. Shimoda, K. Shimode, R. Shink, H. Shinkai, T. Shishido, A. Shoda, D. H. Shoemaker, D. M. Shoemaker, S. ShyamSundar, K. Siellez, M. Sieniawska, D. Sigg, A. D. Silva, L. P. Singer, N. Singh, A. Singhal, A. M. Sintes, S. Sitmukhambetov, V. Skliris, B. J. J. Slagmolen, T. J. Slaven-Blair, J. R. Smith, R. J. E. Smith, S. Somala, K. Somiya, E. J. Son, B. Sorazu, F. Sorrentino, H. Sotani, T. Souradeep, E. Sowell, A. P. Spencer, A. K. Srivastava, V. Srivastava, K. Staats, C. Stachie, M. Standke, D. A. Steer, M. Steinke, J. Steinlechner, S. Steinlechner, D. Steinmeyer, S. P. Stevenson, D. Stocks, R. Stone, D. J. Stops, K. A. Strain, G. Stratta, S. E. Strigin, A. Strunk, R. Sturani, A. L. Stuver, V. Sudhir, R. Sugimoto, T. Z. Summerscales, L. Sun, S. Sunil, J. Suresh, P. J. Sutton, Takamasa Suzuki, Toshikazu Suzuki, B. L. Swinkels, M. J. Szczepańczyk, M. Tacca, H. Tagoshi, S. C. Tait, H. Takahashi, R. Takahashi, A. Takamori, S. Takano, H. Takeda, M. Takeda, C. Talbot, D. Talukder, H. Tanaka, Kazuyuki Tanaka, Kenta Tanaka, Taiki Tanaka, Takahiro Tanaka, S. Tanioka, D. B. Tanner, M. Tápai, E. N. Tapia San Martin, A. Taracchini, J. D. Tasson, R. Taylor, S. Telada, F. Thies, M. Thomas, P. Thomas, S. R. Thondapu, K. A. Thorne, E. Thrane, Shubhanshu Tiwari, Srishti Tiwari, V. Tiwari, K. Toland, T. Tomaru, Y. Tomigami, T. Tomura, M. Tonelli, Z. Tornasi, A. Torres-Forné, C. I. Torrie, D. Töyrä, F. Travasso, G. Traylor, M. C. Tringali, A. Trovato, L. Trozzo, R. Trudeau, K. W. Tsang, T. T. L. Tsang, M. Tse, R. Tso, K. Tsubono, S. Tsuchida, L. Tsukada, D. Tsuna, T. Tsuzuki, D. Tuyenbayev, N. Uchikata, T. Uchiyama, A. Ueda, T. Uehara, K. Ueno, G. Ueshima, D. Ugolini, C. S. Unnikrishnan, F. Uraguchi, A. L. Urban, T. Ushiba, S. A. Usman, H. Vahlbruch, G. Vajente, G. Valdes, N. van Bakel, M. van Beuzekom, J. F. J. van den Brand, C. Van Den Broeck, D. C. Vander-Hyde, L. van der Schaaf, J. V. van Heijningen, M. H. P. M. van Putten, A. A. van Veggel, M. Vardaro, V. Varma, S. Vass, M. Vasúth, A. Vecchio, G. Vedovato, J. Veitch, P. J. Veitch, K. Venkateswara, G. Venugopalan, D. Verkindt, F. Vetrano, A. Viceré, A. D. Viets, D. J. Vine, J.-Y. Vinet, S. Vitale, Francisco Hernandez Vivanco, T. Vo, H. Vocca, C. Vorvick, S. P. Vyatchanin, A. R. Wade, L. E. Wade, M. Wade, R. Walet, M. Walker, L. Wallace, S. Walsh, G. Wang, H. Wang, J. Wang, J. Z. Wang, W. H. Wang, Y. F. Wang, R. L. Ward, Z. A. Warden, J. Warner, M. Was, J. Watchi, B. Weaver, L.-W. Wei, M. Weinert, A. J. Weinstein, R. Weiss, F. Wellmann, L. Wen, E. K. Wessel, P. Weßels, J. W. Westhouse, K. Wette, J. T. Whelan, B. F. Whiting, C. Whittle, D. M. Wilken, D. Williams, A. R. Williamson, J. L. Willis, B. Willke, M. H. Wimmer, W. Winkler, C. C. Wipf, H. Wittel, G. Woan, J. Woehler, J. K. Wofford, J. Worden, J. L. Wright, C. M. Wu, D. S. Wu, H. C. Wu, S. R. Wu, D. M. Wysocki, L. Xiao, W. R. Xu, T. Yamada, H. Yamamoto, Kazuhiro Yamamoto, Kohei Yamamoto, T. Yamamoto, C. C. Yancey, L. Yang, M. J. Yap, M. Yazback, D. W. Yeeles, K. Yokogawa, J. Yokoyama, T. Yokozawa, T. Yoshioka, Hang Yu, Haocun Yu, S. H. R. Yuen, H. Yuzurihara, M. Yvert, A. K. Zadrożny, M. Zanolin, S. Zeidler, T. Zelenova, J.-P. Zendri, M. Zevin, J. Zhang, L. Zhang, T. Zhang, C. Zhao, Y. Zhao, M. Zhou, Z. Zhou, X. J. Zhu, Z. H. Zhu, A. B. Zimmerman, M. E. Zucker, J. Zweizig

    Living Reviews in Relativity   23 ( 1 )   3 - 3   2020.12( ISSN:2367-3613 ( eISSN:1433-8351

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    Publishing type:Research paper (scientific journal)   International / domestic magazine:International journal  

    <title>Abstract</title>We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals for the third (O3), fourth (O4) and fifth observing (O5) runs, including the planned upgrades of the Advanced LIGO and Advanced Virgo detectors. We study the capability of the network to determine the sky location of the source for gravitational-wave signals from the inspiral of binary systems of compact objects, that is binary neutron star, neutron star–black hole, and binary black hole systems. The ability to localize the sources is given as a sky-area probability, luminosity distance, and comoving volume. The median sky localization area (90% credible region) is expected to be a few hundreds of square degrees for all types of binary systems during O3 with the Advanced LIGO and Virgo (HLV) network. The median sky localization area will improve to a few tens of square degrees during O4 with the Advanced LIGO, Virgo, and KAGRA (HLVK) network. During O3, the median localization volume (90% credible region) is expected to be on the order of <inline-formula><alternatives><tex-math>$$10^{5}, 10^{6}, 10^{7}\mathrm {\ Mpc}^3$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:mrow>
    <mml:msup>
    <mml:mn>10</mml:mn>
    <mml:mn>5</mml:mn>
    </mml:msup>
    <mml:mo>,</mml:mo>
    <mml:msup>
    <mml:mn>10</mml:mn>
    <mml:mn>6</mml:mn>
    </mml:msup>
    <mml:mo>,</mml:mo>
    <mml:msup>
    <mml:mn>10</mml:mn>
    <mml:mn>7</mml:mn>
    </mml:msup>
    <mml:msup>
    <mml:mrow>
    <mml:mspace />
    <mml:mi>Mpc</mml:mi>
    </mml:mrow>
    <mml:mn>3</mml:mn>
    </mml:msup>
    </mml:mrow>
    </mml:math></alternatives></inline-formula> for binary neutron star, neutron star–black hole, and binary black hole systems, respectively. The localization volume in O4 is expected to be about a factor two smaller than in O3. We predict a detection count of <inline-formula><alternatives><tex-math>$$1^{+12}_{-1}$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:msubsup>
    <mml:mn>1</mml:mn>
    <mml:mrow>
    <mml:mo>-</mml:mo>
    <mml:mn>1</mml:mn>
    </mml:mrow>
    <mml:mrow>
    <mml:mo>+</mml:mo>
    <mml:mn>12</mml:mn>
    </mml:mrow>
    </mml:msubsup>
    </mml:math></alternatives></inline-formula>(<inline-formula><alternatives><tex-math>$$10^{+52}_{-10}$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:msubsup>
    <mml:mn>10</mml:mn>
    <mml:mrow>
    <mml:mo>-</mml:mo>
    <mml:mn>10</mml:mn>
    </mml:mrow>
    <mml:mrow>
    <mml:mo>+</mml:mo>
    <mml:mn>52</mml:mn>
    </mml:mrow>
    </mml:msubsup>
    </mml:math></alternatives></inline-formula>) for binary neutron star mergers, of <inline-formula><alternatives><tex-math>$$0^{+19}_{-0}$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:msubsup>
    <mml:mn>0</mml:mn>
    <mml:mrow>
    <mml:mo>-</mml:mo>
    <mml:mn>0</mml:mn>
    </mml:mrow>
    <mml:mrow>
    <mml:mo>+</mml:mo>
    <mml:mn>19</mml:mn>
    </mml:mrow>
    </mml:msubsup>
    </mml:math></alternatives></inline-formula>(<inline-formula><alternatives><tex-math>$$1^{+91}_{-1}$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:msubsup>
    <mml:mn>1</mml:mn>
    <mml:mrow>
    <mml:mo>-</mml:mo>
    <mml:mn>1</mml:mn>
    </mml:mrow>
    <mml:mrow>
    <mml:mo>+</mml:mo>
    <mml:mn>91</mml:mn>
    </mml:mrow>
    </mml:msubsup>
    </mml:math></alternatives></inline-formula>) for neutron star–black hole mergers, and <inline-formula><alternatives><tex-math>$$17^{+22}_{-11}$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:msubsup>
    <mml:mn>17</mml:mn>
    <mml:mrow>
    <mml:mo>-</mml:mo>
    <mml:mn>11</mml:mn>
    </mml:mrow>
    <mml:mrow>
    <mml:mo>+</mml:mo>
    <mml:mn>22</mml:mn>
    </mml:mrow>
    </mml:msubsup>
    </mml:math></alternatives></inline-formula>(<inline-formula><alternatives><tex-math>$$79^{+89}_{-44}$$</tex-math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML">
    <mml:msubsup>
    <mml:mn>79</mml:mn>
    <mml:mrow>
    <mml:mo>-</mml:mo>
    <mml:mn>44</mml:mn>
    </mml:mrow>
    <mml:mrow>
    <mml:mo>+</mml:mo>
    <mml:mn>89</mml:mn>
    </mml:mrow>
    </mml:msubsup>
    </mml:math></alternatives></inline-formula>) for binary black hole mergers in a one-calendar-year observing run of the HLV network during O3 (HLVK network during O4). We evaluate sensitivity and localization expectations for unmodeled signal searches, including the search for intermediate mass black hole binary mergers.

    DOI: 10.1007/s41114-020-00026-9

    PubMed

    Other URL: http://link.springer.com/article/10.1007/s41114-020-00026-9/fulltext.html

  • Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA Reviewed

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    LIVING REVIEWS IN RELATIVITY   23 ( 1 )   2020.09( ISSN:2367-3613

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1007/s41114-020-00026-9

  • Overview of KAGRA: Detector design and construction history Reviewed

    T Akutsu,M Ando,K Arai,Y Arai,S Araki,A Araya,N Aritomi,Y Aso,S Bae,Y Bae,L Baiotti,R Bajpai,M A Barton,K Cannon,E Capocasa,M Chan,C Chen,K Chen,Y Chen,H Chu,Y -K Chu,S Eguchi,Y Enomoto,R Flaminio,Y Fujii,M Fukunaga,M Fukushima,G Ge,A Hagiwara,S Haino,K Hasegawa,H Hayakawa,K Hayama,Y Himemoto,Y Hiranuma,N Hirata,E Hirose,Z Hong,B H Hsieh,C -Z Huang,P Huang,Y Huang,B Ikenoue,S Imam,K Inayoshi,Y Inoue,K Ioka,Y Itoh,K Izumi,K Jung,P Jung,T Kajita,M Kamiizumi,N Kanda,G Kang,K Kawaguchi,N Kawai,T Kawasaki,C Kim,J C Kim,W S Kim,Y -M Kim,N Kimura,N Kita,H Kitazawa,Y Kojima,K Kokeyama,K Komori,A K H Kong,K Kotake,C Kozakai,R Kozu,R Kumar,J Kume,C Kuo,H -S Kuo,S Kuroyanagi,K Kusayanagi,K Kwak,H K Lee,H W Lee,R Lee,M Leonardi,L C -C Lin,C -Y Lin,F -L Lin,G C Liu,L -W Luo,M Marchio,Y Michimura,N Mio,O Miyakawa,A Miyamoto,Y Miyazaki,K Miyo,S Miyoki,S Morisaki,Y Moriwaki,K Nagano,S Nagano,K Nakamura,H Nakano,M Nakano,R Nakashima,T Narikawa,R Negishi,W -T Ni,A Nishizawa,Y Obuchi,W Ogaki,J J Oh,S H Oh,M Ohashi,N Ohishi,M Ohkawa,K Okutomi,K Oohara,C P Ooi,S Oshino,K Pan,H Pang,J Park,F E Peña Arellano,I Pinto,N Sago,S Saito,Y Saito,K Sakai,Y Sakai,Y Sakuno,S Sato,T Sato,T Sawada,T Sekiguchi,Y Sekiguchi,S Shibagaki,R Shimizu,T Shimoda,K Shimode,H Shinkai,T Shishido,A Shoda,K Somiya,E J Son,H Sotani,R Sugimoto,T Suzuki,T Suzuki,H Tagoshi,H Takahashi,R Takahashi,A Takamori,S Takano,H Takeda,M Takeda,H Tanaka,K Tanaka,K Tanaka,T Tanaka,T Tanaka,S Tanioka,E N Tapia San Martin,S Telada,T Tomaru,Y Tomigami,T Tomura,F Travasso,L Trozzo,T Tsang,K Tsubono,S Tsuchida,T Tsuzuki,D Tuyenbayev,N Uchikata,T Uchiyama,A Ueda,T Uehara,K Ueno,G Ueshima,F Uraguchi,T Ushiba,M H P M van Putten,H Vocca,J Wang,C Wu,H Wu,S Wu,W- R Xu,T Yamada,K Yamamoto,K Yamamoto,T Yamamoto,K Yokogawa,J Yokoyama,T Yokozawa,T Yoshioka,H Yuzurihara,S Zeidler,Y Zhao,Z -H Zhu

    Progress of Theoretical and Experimental Physics   2020.08

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    DOI: 10.1093/ptep/ptaa125

  • Overview of KAGRA: Detector design and construction history Reviewed

    T Akutsu, M Ando, K Arai, Y Arai, S Araki, A Araya, N Aritomi, Y Aso, S Bae, Y Bae, L Baiotti, R Bajpai, M A Barton, K Cannon, E Capocasa, M Chan, C Chen, K Chen, Y Chen, H Chu, Y -K Chu, S Eguchi, Y Enomoto, R Flaminio, Y Fujii, M Fukunaga, M Fukushima, G Ge, A Hagiwara, S Haino, K Hasegawa, H Hayakawa, K Hayama, Y Himemoto, Y Hiranuma, N Hirata, E Hirose, Z Hong, B H Hsieh, C -Z Huang, P Huang, Y Huang, B Ikenoue, S Imam, K Inayoshi, Y Inoue, K Ioka, Y Itoh, K Izumi, K Jung, P Jung, T Kajita, M Kamiizumi, N Kanda, G Kang, K Kawaguchi, N Kawai, T Kawasaki, C Kim, J C Kim, W S Kim, Y -M Kim, N Kimura, N Kita, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A K H Kong, K Kotake, C Kozakai, R Kozu, R Kumar, J Kume, C Kuo, H -S Kuo, S Kuroyanagi, K Kusayanagi, K Kwak, H K Lee, H W Lee, R Lee, M Leonardi, L C -C Lin, C -Y Lin, F -L Lin, G C Liu, L -W Luo, M Marchio, Y Michimura, N Mio, O Miyakawa, A Miyamoto, Y Miyazaki, K Miyo, S Miyoki, S Morisaki, Y Moriwaki, K Nagano, S Nagano, K Nakamura, H Nakano, M Nakano, R Nakashima, T Narikawa, R Negishi, W -T Ni, A Nishizawa, Y Obuchi, W Ogaki, J J Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, K Okutomi, K Oohara, C P Ooi, S Oshino, K Pan, H Pang, J Park, F E Peña Arellano, I Pinto, N Sago, S Saito, Y Saito, K Sakai, Y Sakai, Y Sakuno, S Sato, T Sato, T Sawada, T Sekiguchi, Y Sekiguchi, S Shibagaki, R Shimizu, T Shimoda, K Shimode, H Shinkai, T Shishido, A Shoda, K Somiya, E J Son, H Sotani, R Sugimoto, T Suzuki, T Suzuki, H Tagoshi, H Takahashi, R Takahashi, A Takamori, S Takano, H Takeda, M Takeda, H Tanaka, K Tanaka, K Tanaka, T Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, S Telada, T Tomaru, Y Tomigami, T Tomura, F Travasso, L Trozzo, T Tsang, K Tsubono, S Tsuchida, T Tsuzuki, D Tuyenbayev, N Uchikata, T Uchiyama, A Ueda, T Uehara, K Ueno, G Ueshima, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, J Wang, C Wu, H Wu, S Wu, W- R Xu, T Yamada, K Yamamoto, K Yamamoto, T Yamamoto, K Yokogawa, J Yokoyama, T Yokozawa, T Yoshioka, H Yuzurihara, S Zeidler, Y Zhao, Z -H Zhu

    Progress of Theoretical and Experimental Physics   2021 ( 5 )   2020.08( eISSN:2050-3911

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    <title>Abstract</title>
    KAGRA is a newly built gravitational-wave telescope, a laser interferometer comprising arms with a length of 3 km, located in Kamioka, Gifu, Japan. KAGRA was constructed under the ground and it is operated using cryogenic mirrors that help in reducing the seismic and thermal noise. Both technologies are expected to provide directions for the future of gravitational-wave telescopes. In 2019, KAGRA finished all installations with the designed configuration, which we call the baseline KAGRA. For this occasion, we present an overview of the baseline KAGRA from various viewpoints in a series of articles. In this article, we introduce the design configurations of KAGRA with its historical background.

    DOI: 10.1093/ptep/ptaa125

  • Overview of KAGRA: KAGRA science Reviewed

    T Akutsu,M Ando,K Arai,Y Arai,S Araki,A Araya,N Aritomi,H Asada,Y Aso,S Bae,Y Bae,L Baiotti,R Bajpai,M A Barton,K Cannon,Z Cao,E Capocasa,M Chan,C Chen,K Chen,Y Chen,C -Y Chiang,H Chu,Y -K Chu,S Eguchi,Y Enomoto,R Flaminio,Y Fujii,F Fujikawa,M Fukunaga,M Fukushima,D Gao,G Ge,S Ha,A Hagiwara,S Haino,W -B Han,K Hasegawa,K Hattori,H Hayakawa,K Hayama,Y Himemoto,Y Hiranuma,N Hirata,E Hirose,Z Hong,B H Hsieh,C -Z Huang,H -Y Huang,P Huang,Y Huang,Y -C Huang,D C Y Hui,S Ide,B Ikenoue,S Imam,K Inayoshi,Y Inoue,K Ioka,K Ito,Y Itoh,K Izumi,C Jeon,H -B Jin,K Jung,P Jung,K Kaihotsu,T Kajita,M Kakizaki,M Kamiizumi,N Kanda,G Kang,K Kashiyama,K Kawaguchi,N Kawai,T Kawasaki,C Kim,J Kim,J C Kim,W S Kim,Y -M Kim,N Kimura,N Kita,H Kitazawa,Y Kojima,K Kokeyama,K Komori,A K H Kong,K Kotake,C Kozakai,R Kozu,R Kumar,J Kume,C Kuo,H -S Kuo,Y Kuromiya,S Kuroyanagi,K Kusayanagi,K Kwak,H K Lee,H W Lee,R Lee,M Leonardi,K L Li,T G F Li,C -Y Lin,F -K Lin,F -L Lin,H L Lin,L C -C Lin,G C Liu,L -W Luo,E Majorana,M Marchio,Y Michimura,N Mio,O Miyakawa,A Miyamoto,Y Miyazaki,K Miyo,S Miyoki,Y Mori,S Morisaki,Y Moriwaki,K Nagano,S Nagano,K Nakamura,H Nakano,M Nakano,R Nakashima,Y Nakayama,T Narikawa,L Naticchioni,R Negishi,L Nguyen Quynh,W -T Ni,A Nishizawa,S Nozaki,Y Obuchi,W Ogaki,J J Oh,K Oh,S H Oh,M Ohashi,N Ohishi,M Ohkawa,H Ohta,Y Okutani,K Okutomi,K Oohara,C P Ooi,S Oshino,S Otabe,K Pan,H Pang,A Parisi,J Park,F E Pe na Arellano,I Pinto,N Sago,S Saito,Y Saito,K Sakai,Y Sakai,Y Sakuno,S Sato,T Sato,T Sawada,T Sekiguchi,Y Sekiguchi,L Shao,S Shibagaki,R Shimizu,T Shimoda,K Shimode,H Shinkai,T Shishido,A Shoda,K Somiya,E J Son,H Sotani,R Sugimoto,J Suresh,T Suzuki,T Suzuki,H Tagoshi,H Takahashi,R Takahashi,A Takamori,S Takano,H Takeda,M Takeda,H Tanaka,K Tanaka,K Tanaka,T Tanaka,T Tanaka,S Tanioka,E N Tapia San Martin,S Telada,T Tomaru,Y Tomigami,T Tomura,F Travasso,L Trozzo,T Tsang,J -S Tsao,K Tsubono,S Tsuchida,D Tsuna,T Tsutsui,T Tsuzuki,D Tuyenbayev,N Uchikata,T Uchiyama,A Ueda,T Uehara,K Ueno,G Ueshima,F Uraguchi,T Ushiba,M H P M van Putten,H Vocca,J Wang,T Washimi,C Wu,H Wu,S Wu,W -R Xu,T Yamada,K Yamamoto,K Yamamoto,T Yamamoto,K Yamashita,R Yamazaki,Y Yang,K Yokogawa,J Yokoyama,T Yokozawa,T Yoshioka,H Yuzurihara,S Zeidler,M Zhan,H Zhang,Y Zhao,Z -H Zhu

    Progress of Theoretical and Experimental Physics   2020.08

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  • Overview of KAGRA: KAGRA science

    T Akutsu, M Ando, K Arai, Y Arai, S Araki, A Araya, N Aritomi, H Asada, Y Aso, S Bae, Y Bae, L Baiotti, R Bajpai, M A Barton, K Cannon, Z Cao, E Capocasa, M Chan, C Chen, K Chen, Y Chen, C -Y Chiang, H Chu, Y -K Chu, S Eguchi, Y Enomoto, R Flaminio, Y Fujii, F Fujikawa, M Fukunaga, M Fukushima, D Gao, G Ge, S Ha, A Hagiwara, S Haino, W -B Han, K Hasegawa, K Hattori, H Hayakawa, K Hayama, Y Himemoto, Y Hiranuma, N Hirata, E Hirose, Z Hong, B H Hsieh, C -Z Huang, H -Y Huang, P Huang, Y Huang, Y -C Huang, D C Y Hui, S Ide, B Ikenoue, S Imam, K Inayoshi, Y Inoue, K Ioka, K Ito, Y Itoh, K Izumi, C Jeon, H -B Jin, K Jung, P Jung, K Kaihotsu, T Kajita, M Kakizaki, M Kamiizumi, N Kanda, G Kang, K Kashiyama, K Kawaguchi, N Kawai, T Kawasaki, C Kim, J Kim, J C Kim, W S Kim, Y -M Kim, N Kimura, N Kita, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A K H Kong, K Kotake, C Kozakai, R Kozu, R Kumar, J Kume, C Kuo, H -S Kuo, Y Kuromiya, S Kuroyanagi, K Kusayanagi, K Kwak, H K Lee, H W Lee, R Lee, M Leonardi, K L Li, T G F Li, C -Y Lin, F -K Lin, F -L Lin, H L Lin, L C -C Lin, G C Liu, L -W Luo, E Majorana, M Marchio, Y Michimura, N Mio, O Miyakawa, A Miyamoto, Y Miyazaki, K Miyo, S Miyoki, Y Mori, S Morisaki, Y Moriwaki, K Nagano, S Nagano, K Nakamura, H Nakano, M Nakano, R Nakashima, Y Nakayama, T Narikawa, L Naticchioni, R Negishi, L Nguyen Quynh, W -T Ni, A Nishizawa, S Nozaki, Y Obuchi, W Ogaki, J J Oh, K Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, H Ohta, Y Okutani, K Okutomi, K Oohara, C P Ooi, S Oshino, S Otabe, K Pan, H Pang, A Parisi, J Park, F E Pe na Arellano, I Pinto, N Sago, S Saito, Y Saito, K Sakai, Y Sakai, Y Sakuno, S Sato, T Sato, T Sawada, T Sekiguchi, Y Sekiguchi, L Shao, S Shibagaki, R Shimizu, T Shimoda, K Shimode, H Shinkai, T Shishido, A Shoda, K Somiya, E J Son, H Sotani, R Sugimoto, J Suresh, T Suzuki, T Suzuki, H Tagoshi, H Takahashi, R Takahashi, A Takamori, S Takano, H Takeda, M Takeda, H Tanaka, K Tanaka, K Tanaka, T Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, S Telada, T Tomaru, Y Tomigami, T Tomura, F Travasso, L Trozzo, T Tsang, J -S Tsao, K Tsubono, S Tsuchida, D Tsuna, T Tsutsui, T Tsuzuki, D Tuyenbayev, N Uchikata, T Uchiyama, A Ueda, T Uehara, K Ueno, G Ueshima, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, J Wang, T Washimi, C Wu, H Wu, S Wu, W -R Xu, T Yamada, K Yamamoto, K Yamamoto, T Yamamoto, K Yamashita, R Yamazaki, Y Yang, K Yokogawa, J Yokoyama, T Yokozawa, T Yoshioka, H Yuzurihara, S Zeidler, M Zhan, H Zhang, Y Zhao, Z -H Zhu

    Oxford University Press (OUP) Progress of Theoretical and Experimental Physics   2021 ( 5 )   2020.08( ISSN:2050-3911

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    <title>Abstract</title>
    KAGRA is a newly build gravitational wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring KAGRA, we discuss the science targets of KAGRA projects, considering not only the baseline KAGRA (current design) but also its future upgrade candidates (KAGRA+) for the near to middle term ($\sim$5 years).

    DOI: 10.1093/ptep/ptaa120

  • Overview of KAGRA: KAGRA science Reviewed

    T Akutsu, M Ando, K Arai, Y Arai, S Araki, A Araya, N Aritomi, H Asada, Y Aso, S Bae, Y Bae, L Baiotti, R Bajpai, M A Barton, K Cannon, Z Cao, E Capocasa, M Chan, C Chen, K Chen, Y Chen, C -Y Chiang, H Chu, Y -K Chu, S Eguchi, Y Enomoto, R Flaminio, Y Fujii, F Fujikawa, M Fukunaga, M Fukushima, D Gao, G Ge, S Ha, A Hagiwara, S Haino, W -B Han, K Hasegawa, K Hattori, H Hayakawa, K Hayama, Y Himemoto, Y Hiranuma, N Hirata, E Hirose, Z Hong, B H Hsieh, C -Z Huang, H -Y Huang, P Huang, Y Huang, Y -C Huang, D C Y Hui, S Ide, B Ikenoue, S Imam, K Inayoshi, Y Inoue, K Ioka, K Ito, Y Itoh, K Izumi, C Jeon, H -B Jin, K Jung, P Jung, K Kaihotsu, T Kajita, M Kakizaki, M Kamiizumi, N Kanda, G Kang, K Kashiyama, K Kawaguchi, N Kawai, T Kawasaki, C Kim, J Kim, J C Kim, W S Kim, Y -M Kim, N Kimura, N Kita, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A K H Kong, K Kotake, C Kozakai, R Kozu, R Kumar, J Kume, C Kuo, H -S Kuo, Y Kuromiya, S Kuroyanagi, K Kusayanagi, K Kwak, H K Lee, H W Lee, R Lee, M Leonardi, K L Li, T G F Li, C -Y Lin, F -K Lin, F -L Lin, H L Lin, L C -C Lin, G C Liu, L -W Luo, E Majorana, M Marchio, Y Michimura, N Mio, O Miyakawa, A Miyamoto, Y Miyazaki, K Miyo, S Miyoki, Y Mori, S Morisaki, Y Moriwaki, K Nagano, S Nagano, K Nakamura, H Nakano, M Nakano, R Nakashima, Y Nakayama, T Narikawa, L Naticchioni, R Negishi, L Nguyen Quynh, W -T Ni, A Nishizawa, S Nozaki, Y Obuchi, W Ogaki, J J Oh, K Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, H Ohta, Y Okutani, K Okutomi, K Oohara, C P Ooi, S Oshino, S Otabe, K Pan, H Pang, A Parisi, J Park, F E Pe na Arellano, I Pinto, N Sago, S Saito, Y Saito, K Sakai, Y Sakai, Y Sakuno, S Sato, T Sato, T Sawada, T Sekiguchi, Y Sekiguchi, L Shao, S Shibagaki, R Shimizu, T Shimoda, K Shimode, H Shinkai, T Shishido, A Shoda, K Somiya, E J Son, H Sotani, R Sugimoto, J Suresh, T Suzuki, T Suzuki, H Tagoshi, H Takahashi, R Takahashi, A Takamori, S Takano, H Takeda, M Takeda, H Tanaka, K Tanaka, K Tanaka, T Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, S Telada, T Tomaru, Y Tomigami, T Tomura, F Travasso, L Trozzo, T Tsang, J -S Tsao, K Tsubono, S Tsuchida, D Tsuna, T Tsutsui, T Tsuzuki, D Tuyenbayev, N Uchikata, T Uchiyama, A Ueda, T Uehara, K Ueno, G Ueshima, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, J Wang, T Washimi, C Wu, H Wu, S Wu, W -R Xu, T Yamada, K Yamamoto, K Yamamoto, T Yamamoto, K Yamashita, R Yamazaki, Y Yang, K Yokogawa, J Yokoyama, T Yokozawa, T Yoshioka, H Yuzurihara, S Zeidler, M Zhan, H Zhang, Y Zhao, Z -H Zhu

    Progress of Theoretical and Experimental Physics   2021 ( 5 )   2020.08( eISSN:2050-3911

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    Publishing type:Research paper (scientific journal)  

    <title>Abstract</title>
    KAGRA is a newly build gravitational wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring KAGRA, we discuss the science targets of KAGRA projects, considering not only the baseline KAGRA (current design) but also its future upgrade candidates (KAGRA+) for the near to middle term ($\sim$5 years).

    DOI: 10.1093/ptep/ptaa120

  • Application of independent component analysis to the iKAGRA data

    T. Akutsu, T. Akutsu, M. Ando, M. Ando, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya, N. Aritomi, H. Asada, H. Asada, Y. Aso, Y. Aso, S. Atsuta, K. Awai, S. Bae, Y. Bae, L. Baiotti, R. Bajpai, M. A. Barton, K. Cannon, E. Capocasa, M. Chan, C. Chen, C. Chen, K. Chen, Y. Chen, H. Chu, Y. K. Chu, K. Craig, W. Creus, K. Doi, K. Eda, S. Eguchi, Y. Enomoto, R. Flaminio, R. Flaminio, Y. Fujii, M. K. Fujimoto, M. Fukunaga, M. Fukushima, T. Furuhata, G. Ge, A. Hagiwara, A. Hagiwara, S. Haino, K. Hasegawa, K. Hashino, H. Hayakawa, K. Hayama, Y. Himemoto, Y. Hiranuma, N. Hirata, S. Hirobayashi, E. Hirose, Z. Hong, B. H. Hsieh, G. Z. Huang, P. Huang, Y. Huang, B. Ikenoue, S. Imam, K. Inayoshi, Y. Inoue, K. Ioka, Y. Itoh, Y. Itoh, K. Izumi, K. Jung, P. Jung, T. Kaji, T. Kajita, M. Kakizaki, M. Kamiizumi, S. Kanbara, N. Kanda, N. Kanda, S. Kanemura, M. Kaneyama, G. Kang, J. Kasuya, Y. Kataoka, K. Kawaguchi, N. Kawai, S. Kawamura, T. Kawasaki, C. Kim, J. C. Kim, W. S. Kim, Y. M. Kim, N. Kimura, T. Kinugawa, S. Kirii, N. Kita, Y. Kitaoka, H. Kitazawa, Y. Kojima, K. Kokeyama, K. Komori

    Progress of Theoretical and Experimental Physics   2020 ( 5 )   2020.05( eISSN:2050-3911

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    We apply independent component analysis (ICA) to real data from a gravitational wave detector for the first time. Specifically, we use the iKAGRA data taken in April 2016, and calculate the correlations between the gravitational wave strain channel and 35 physical environmental channels. Using a couple of seismic channels which are found to be strongly correlated with the strain, we perform ICA. Injecting a sinusoidal continuous signal in the strain channel, we find that ICA recovers correct parameters with enhanced signal-to-noise ratio, which demonstrates the usefulness of this method. Among the two implementations of ICA used here, we find the correlation method yields the optimal results for the case of environmental noise acting on the strain channel linearly.

    DOI: 10.1093/ptep/ptaa056

  • Application of independent component analysis to the iKAGRA data Reviewed

    Akutsu T., Ando M., Arai K., Arai Y., Araki S., Araya A., Aritomi N., Asada H., Aso Y., Atsuta S., Awai K., Bae S., Bae Y., Baiotti L., Bajpai R., Barton M. A., Cannon K., Capocasa E., Chan M., Chen C., Chen K., Chen Y., Chu H., Chu Y-K, Craig K., Creus W., Doi K., Eda K., Eguchi S., Enomoto Y., Flaminio R., Fujii Y., Fujimoto M-K, Fukunaga M., Fukushima M., Furuhata T., Ge G., Hagiwara A., Haino S., Hasegawa K., Hashino K., Hayakawa H., Hayama K., Himemoto Y., Hiranuma Y., Hirata N., Hirobayashi S., Hirose E., Hong Z., Hsieh B. H., Huang G-Z, Huang P., Huang Y., Ikenoue B., Imam S., Inayoshi K., Inoue Y., Ioka K., Itoh Y., Izumi K., Jung K., Jung P., Kaji T., Kajita T., Kakizaki M., Kamiizumi M., Kanbara S., Kanda N., Kanemura S., Kaneyama M., Kang G., Kasuya J., Kataoka Y., Kawaguchi K., Kawai N., Kawamura S., Kawasaki T., Kim C., Kim J. C., Kim W. S., Kim Y-M, Kimura N., Kinugawa T., Kirii S., Kita N., Kitaoka Y., Kitazawa H., Kojima Y., Kokeyama K., Komori K., Kong A. K. H., Kotake K., Kozakai C., Kozu R., Kumar R., Kume J., Kuo C., Kuo H-S, Kuroyanagi S., Kusayanagi K., Kwak K., Lee H. K., Lee H. M., Lee H. W., Lee R., Leonardi M., Lin C., Lin C-Y, Lin F-L, Liu G. C., Liu Y., Luo L., Majorana E., Mano S., Marchio M., Matsui T., Matsushima F., Michimura Y., Mio N., Miyakawa O., Miyamoto A., Miyamoto T., Miyazaki Y., Miyo K., Miyoki S., Morii W., Morisaki S., Moriwaki Y., Morozumi T., Musha M., Nagano K., Nagano S., Nakamura K., Nakamura T., Nakano H., Nakano M., Nakao K., Nakashima R., Narikawa T., Naticchioni L., Negishi R., NguyenQuynh L., Ni W-T, Nishizawa A., Obuchi Y., Ochi T., Ogaki W., Oh J. J., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Okutomi K., Oohara K., Ooi C. P., Oshino S., Pan K., Pang H., Park J., Arellano F. E. Pena, Pinto I, Sago N., Saijo M., Saito S., Saito Y., Sakai K., Sakai Y., Sakai Y., Sakuno Y., Sasaki M., Sasaki Y., Sato S., Sato T., Sawada T., Sekiguchi T., Sekiguchi Y., Seto N., Shibagaki S., Shibata M., Shimizu R., Shimoda T., Shimode K., Shinkai H., Shishido T., Shoda A., Somiya K., Son E. J., Sotani H., Suemasa A., Sugimoto R., Suzuki T., Suzuki T., Tagoshi H., Takahashi H., Takahashi R., Takamori A., Takano S., Takeda H., Takeda M., Tanaka H., Tanaka K., Tanaka K., Tanaka T., Tanaka T., Tanioka S., San Martin E. N. Tapia, Tatsumi D., Telada S., Tomaru T., Tomigami Y., Tomura T., Travasso F., Trozzo L., Tsang T., Tsubono K., Tsuchida S., Tsuzuki T., Tuyenbayev D., Uchikata N., Uchiyama T., Ueda A., Uehara T., Ueki S., Ueno K., Ueshima G., Uraguchi F., Ushiba T., van Putten M. H. P. M., Vocca H., Wada S., Wakamatsu T., Wang J., Wu C., Wu H., Wu S., Xu W-R, Yamada T., Yamamoto A., Yamamoto K., Yamamoto K., Yamamoto S., Yamamoto T., Yokogawa K., Yokoyama J., Yokozawa T., Yoon T. H., Yoshioka T., Yuzurihara H., Zeidler S., Zhao Y., Zhu Z-H

    PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS   2020 ( 5 )   2020.05( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptaa056

  • Dark matter signals on laser interferometer

    Tsuchida S.

    Journal of Physics: Conference Series   1468 ( 1 )   2020.03( ISSN:17426588

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    DOI: 10.1088/1742-6596/1468/1/012022

  • Swelling of Doubly Magic Ca 48 Core in Ca Isotopes beyond N=28

    Tanaka M.

    Physical Review Letters   124 ( 10 )   2020.03( ISSN:00319007

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevLett.124.102501

  • An arm length stabilization system for KAGRA and future gravitational-wave detectors Reviewed

    Akutsu T., Ando M., Arai K., Arai Y., Araki S., Araya A., Aritomi N., Aso Y., Bae S., Bae Y., Baiotti L., Bajpai R., Barton M. A., Cannon K., Capocasa E., Chan M., Chen C. S., Chen K., Chen Y., Chu H., Chu Y-K, Doi K., Eguchi S., Enomoto Y., Flaminio R., Fujii Y., Fukunaga M., Fukushima M., Ge G-G, Hagiwara A., Haino S., Hasegawa K., Hayakawa H., Hayama K., Himemoto Y., Hiranuma Y., Hirata N., Hirose E., Hong Z., Hsieh B. H., Huang G-Z, Huang P-W, Huang Y., Ikenoue B., Imam S., Inayoshi K., Inoue Y., Ioka K., Itoh Y., Izumi K., Jung K., Jung P., Kajita T., Kamiizumi M., Kanbara S., Kanda N., Kang G., Kawaguchi K., Kawai N., Kawasaki T., Kim C., Kim J. C., Kim W. S., Kim Y-M, Kimura N., Kita N., Kitazawa H., Kojima Y., Kokeyama K., Komori K., Kong A. K. H., Kotake K., Kozakai C., Kozu R., Kumar R., Kume J., Kuo C., Kuo H-S, Kuroyanagi S., Kusayanagi K., Kwak K., Lee H. K., Lee H. W., Lee R., Leonardi M., Lin L. C-C, Lin C-Y, Lin F-L, Liu G. C., Luo L-W, Marchio M., Michimura Y., Mio N., Miyakawa O., Miyamoto A., Miyazaki Y., Miyo K., Miyoki S., Morisaki S., Moriwaki Y., Musha M., Nagano K., Nagano S., Nakamura K., Nakano H., Nakano M., Nakashima R., Narikawa T., Negishi R., Ni W-T, Nishizawa A., Obuchi Y., Ogaki W., Oh J. J., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Ohmae N., Okutomi K., Oohara K., Ooi C. P., Oshino S., Pan K-C, Pang H., Park J., Arellano F. E. Pena, Pinto I, Sago N., Saito S., Saito Y., Sakai K., Sakai Y., Sakuno Y., Sato S., Sato T., Sawada T., Sekiguchi T., Sekiguchi Y., Shibagaki S., Shimizu R., Shimoda T., Shimode K., Shinkai H., Shishido T., Shoda A., Somiya K., Son E. J., Sotani H., Sugimoto R., Suzuki T., Tagoshi H., Takahashi H., Takahashi R., Takamori A., Takano S., Takeda H., Takeda M., Tanaka H., Tanaka K., Tanaka T., Tanioka S., San Martin E. N. Tapia, Tatsumi D., Telada S., Tomaru T., Tomigami Y., Tomura T., Travasso F., Trozzo L., Tsang T., Tsubono K., Tsuchida S., Tsuzuki T., Tuyenbayev D., Uchikata N., Uchiyama T., Ueda A., Uehara T., Ueno K., Ueshima G., Uraguchi F., Ushiba T., van Putten M. H. P. M., Vocca H., Wang J., Wu C., Wu H., Wu S., Xu W-R, Yamada T., Yamamoto K., Yamamoto T., Yokogawa K., Yokoyama J., Yokozawa T., Yoshioka T., Yuzurihara H., Zeidler S., Zhao Y., Zhu Z-H

    CLASSICAL AND QUANTUM GRAVITY   37 ( 3 )   2020.02( ISSN:0264-9381

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1088/1361-6382/ab5c95

  • An arm length stabilization system for KAGRA and future gravitational-wave detectors Reviewed

    T Akutsu, M Ando, K Arai, K Arai, Y Arai, S Araki, A Araya, N Aritomi, Y Aso, S Bae, Y Bae, L Baiotti, R Bajpai, M A Barton, K Cannon, E Capocasa, M Chan, C S Chen, K Chen, Y Chen, H Chu, Y-K Chu, K Doi, S Eguchi, Y Enomoto, R Flaminio, Y Fujii, M Fukunaga, M Fukushima, G-G Ge, A Hagiwara, S Haino, K Hasegawa, H Hayakawa, K Hayama, Y Himemoto, Y Hiranuma, N Hirata, E Hirose, Z Hong, B H Hsieh, G-Z Huang, P-W Huang, Y Huang, B Ikenoue, S Imam, K Inayoshi, Y Inoue, K Ioka, Y Itoh, K Izumi, K Jung, P Jung, T Kajita, M Kamiizumi, S Kanbara, N Kanda, G Kang, K Kawaguchi, N Kawai, T Kawasaki, C Kim, J C Kim, W S Kim, Y-M Kim, N Kimura, N Kita, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A K H Kong, K Kotake, C Kozakai, R Kozu, R Kumar, J Kume, C Kuo, H-S Kuo, S Kuroyanagi, K Kusayanagi, K Kwak, H K Lee, H W Lee, R Lee, M Leonardi, L C-C Lin, C-Y Lin, F-L Lin, G C Liu, L-W Luo, M Marchio, Y Michimura, N Mio, O Miyakawa, A Miyamoto, Y Miyazaki, K Miyo, S Miyoki, S Morisaki, Y Moriwaki, M Musha, K Nagano, S Nagano, K Nakamura, H Nakano, M Nakano, R Nakashima, T Narikawa, R Negishi, W-T Ni, A Nishizawa, Y Obuchi, W Ogaki, J J Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, N Ohmae, K Okutomi, K Oohara, C P Ooi, S Oshino, K-C Pan, H Pang, J Park, F E Peña Arellano, I Pinto, N Sago, S Saito, Y Saito, K Sakai, Y Sakai, Y Sakuno, S Sato, T Sato, T Sawada, T Sekiguchi, Y Sekiguchi, S Shibagaki, R Shimizu, T Shimoda, K Shimode, H Shinkai, T Shishido, A Shoda, K Somiya, E J Son, H Sotani, R Sugimoto, T Suzuki, T Suzuki, H Tagoshi, H Takahashi, R Takahashi, A Takamori, S Takano, H Takeda, M Takeda, H Tanaka, K Tanaka, K Tanaka, T Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, D Tatsumi, S Telada, T Tomaru, Y Tomigami, T Tomura, F Travasso, L Trozzo, T Tsang, K Tsubono, S Tsuchida, T Tsuzuki, D Tuyenbayev, N Uchikata, T Uchiyama, A Ueda, T Uehara, K Ueno, G Ueshima, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, J Wang, C Wu, H Wu, S Wu, W-R Xu, T Yamada, K Yamamoto, K Yamamoto, T Yamamoto, K Yokogawa, J Yokoyama, T Yokozawa, T Yoshioka, H Yuzurihara, S Zeidler, Y Zhao, Z-H Zhu

    Classical and Quantum Gravity   37 ( 3 )   035004 - 035004   2020.02( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/1361-6382/ab5c95

    Other URL: https://iopscience.iop.org/article/10.1088/1361-6382/ab5c95

  • Dark matter signals on a laser interferometer Reviewed

    Tsuchida Satoshi, Kanda Nobuyuki, Itoh Yousuke, Mori Masaki

    PHYSICAL REVIEW D   101 ( 2 )   2020.01( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.101.023005

  • Dark matter signals on a laser interferometer Reviewed

    Tsuchida Satoshi, Kanda Nobuyuki, Itoh Yousuke, Mori Masaki

    PHYSICAL REVIEW D   101 ( 2 )   2020.01( ISSN:2470-0010 ( eISSN:2470-0029

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    WIMPs are promising dark matter candidates. A WIMP occasionally collides with a mirror equipped with interferometric gravitational wave detectors such as LIGO, Virgo, KAGRA and the Einstein Telescope (ET). When WIMPs collide with a mirror of an interferometer, we expect that characteristic motions of the pendulum and mirror are excited, and those signals could be extracted by highly sophisticated sensors developed for gravitational wave detection. We analyze the motions of the pendulum and mirror, and estimate the detectability of these motions. For the "Thin-ET" detector, the signal-to-noise ratio may be 1.7(m(DM)/100 GeV), where m(DM) is the mass of a WIMP. We may set a more strict upper limit on the cross section between a WIMP and a nucleon than the limits obtained by other experiments so far when m(DM) is approximately lower than 0.2 GeV. We find an order-of-magnitude improvement in the upper limit around m(DM) = 0.2 GeV.

    DOI: 10.1103/PhysRevD.101.023005

  • The status of KAGRA underground cryogenic gravitational wave telescope Reviewed

    T. Akutsu,M. Ando,A. Araya,N. Aritomi,H. Asada,Y. Aso,S. Atsuta,K. Awai,M. A. Barton,K. Cannon,K. Craig,W. Creus,K. Doi,K. Eda,Y. Enomoto,R. Flaminio,Y. Fujii,M.-K. Fujimoto,T. Furuhata,S. Haino,K. Hasegawa,K. Hashino,K. Hayama,S. Hirobayashi,E. Hirose,A. H. Hsieh,Y. Inoue,K. Ioka,Y. Itoh,T. Kaji,T. Kajita,M. Kakizaki,M. Kamiizumi,S. Kambara,N. Kanda,S. Kanemura,M. Kaneyama,G. Kang,J. Kasuya,Y. Kataoka,N. Kawai,S. Kawamura,C. Kim,H. Kim,J. Kim,Y. Kim,N. Kimura,T. Kinugawa,S. Kirii,Y. Kitaoka,Y. Kojima,K. Kokeyama,K. Komori,K. Kotake,R. Kumar,H. Lee,H. Lee,Y. Liu,N. Luca,E. Majorana,S. Mano,M. Marchio,T. Matsui,F. Matsushima,Y. Michimura,O. Miyakawa,T. Miyamoto,A. Miyamoto,K. Miyo,S. Miyoki,W. Morii,S. Morisaki,Y. Moriwaki,T. Morozumi,M. Musha,S. Nagano,K. Nagano,K. Nakamura,T. Nakamura,H. Nakano,M. Nakano,K. Nakao,T. Narikawa,L.Nguyen Quynh,W.-T. Ni,T. Ochi,J. Oh,S. Oh,M. Ohashi,N. Ohishi,M. Ohkawa,K. Okutomi,K. Oohara,F. E.Peña Alleano,I. Pinto,N. Sago,M. Saijo,Y. Saito,K. Sakai,Y. Sakai,Y. Sasaki,M. Sasaki,S. Sato,T. Sato,Y. Sekiguchi,N. Seto,M. Shibata,T. Shimoda,H. Shinkai,A. Shoda,K. Somiya,E. Son,A. Suemasa,T. Suzuki,T. Suzuki,H. Tagoshi,H. Takahashi,R. Takahashi,A. Takamori,H. Takeda,H. Tanaka,K. Tanaka,T. Tanaka,D. Tatsumi,T. Tomaru,T. Tomura,F. Travasso,K. Tsubono,S. Tsuchida,N. Uchikata,T. Uchiyama,T. Uehara,S. Ueki,K. Ueno,T. Ushiba,M. H. P. M. van Putten,H. Vocca,S. Wada,T. Wakamatsu,T. Yamada,S. Yamamoto,T. Yamamoto,K. Yamamoto,A. Yamamoto,J. Yokoyama,T. Yokozawa,T. H. Yoon,H. Yuzurihara,S. Zeidler,Z.-H. Zhu

    Journal of Physics: Conference Series   2020.01

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    The status of KAGRA underground cryogenic gravitational wave telescope

    DOI: 10.1088/1742-6596/1342/1/012014

  • The status of KAGRA underground cryogenic gravitational wave telescope Reviewed

    T. Akutsu, M. Ando, A. Araya, N. Aritomi, H. Asada, Y. Aso, S. Atsuta, K. Awai, M. A. Barton, K. Cannon, K. Craig, W. Creus, K. Doi, K. Eda, Y. Enomoto, R. Flaminio, Y. Fujii, M.-K. Fujimoto, T. Furuhata, S. Haino, K. Hasegawa, K. Hashino, K. Hayama, S. Hirobayashi, E. Hirose, A. H. Hsieh, Y. Inoue, K. Ioka, Y. Itoh, T. Kaji, T. Kajita, M. Kakizaki, M. Kamiizumi, S. Kambara, N. Kanda, S. Kanemura, M. Kaneyama, G. Kang, J. Kasuya, Y. Kataoka, N. Kawai, S. Kawamura, C. Kim, H. Kim, J. Kim, Y. Kim, N. Kimura, T. Kinugawa, S. Kirii, Y. Kitaoka, Y. Kojima, K. Kokeyama, K. Komori, K. Kotake, R. Kumar, H. Lee, H. Lee, Y. Liu, N. Luca, E. Majorana, S. Mano, M. Marchio, T. Matsui, F. Matsushima, Y. Michimura, O. Miyakawa, T. Miyamoto, A. Miyamoto, K. Miyo, S. Miyoki, W. Morii, S. Morisaki, Y. Moriwaki, T. Morozumi, M. Musha, S. Nagano, K. Nagano, K. Nakamura, T. Nakamura, H. Nakano, M. Nakano, K. Nakao, T. Narikawa, L.Nguyen Quynh, W.-T. Ni, T. Ochi, J. Oh, S. Oh, M. Ohashi, N. Ohishi, M. Ohkawa, K. Okutomi, K. Oohara, F. E.Peña Alleano, I. Pinto, N. Sago, M. Saijo, Y. Saito, K. Sakai, Y. Sakai, Y. Sasaki, M. Sasaki, S. Sato, T. Sato, Y. Sekiguchi, N. Seto, M. Shibata, T. Shimoda, H. Shinkai, A. Shoda, K. Somiya, E. Son, A. Suemasa, T. Suzuki, T. Suzuki, H. Tagoshi, H. Takahashi, R. Takahashi, A. Takamori, H. Takeda, H. Tanaka, K. Tanaka, T. Tanaka, D. Tatsumi, T. Tomaru, T. Tomura, F. Travasso, K. Tsubono, S. Tsuchida, N. Uchikata, T. Uchiyama, T. Uehara, S. Ueki, K. Ueno, T. Ushiba, M. H. P. M. van Putten, H. Vocca, S. Wada, T. Wakamatsu, T. Yamada, S. Yamamoto, T. Yamamoto, K. Yamamoto, A. Yamamoto, J. Yokoyama, T. Yokozawa, T. H. Yoon, H. Yuzurihara, S. Zeidler, Z.-H. Zhu

    Journal of Physics: Conference Series   1342 ( 1 )   012014 - 012014   2020.01( ISSN:1742-6588 ( eISSN:1742-6596

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    DOI: 10.1088/1742-6596/1342/1/012014

    Other URL: https://iopscience.iop.org/article/10.1088/1742-6596/1342/1/012014

  • Space gravitational-wave antennas DECIGO and B-DECIGO Reviewed

    Kawamura Seiji, Nakamura Takashi, Ando Masaki, Seto Naoki, Akutsu Tomotada, Funaki Ikkoh, Ioka Kunihito, Kanda Nobuyuki, Kawano Isao, Musha Mitsuru, Nakazawa Kazuhiro, Sato Shuichi, Takashima Takeshi, Tanaka Takahiro, Tsubono Kimio, Yokoyama Jun'ichi, Agatsuma Kazuhiro, Aoyanagi Koh-suke, Arai Koji, Araya Akito, Aritomi Naoki, Asada Hideki, Aso Yoichi, Chen Dan, Chiba Takeshi, Ebisuzaki Toshikazu, Eguchi Satoshi, Ejiri Yumiko, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Gondo Rina, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T., Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Izumi Kiwamu, Kanemura Shinya, Kawashima Nobuki, Kawazoe Fumiko, Kishimoto Naoko, Kiuchi Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Kuroyanagi Sachiko, Maeda Kei-ichi, Matsuhara Hideo, Matsumoto Nobuyuki, Michimura Yuta, Miyakawa Osamu, Miyamoto Umpei, Miyoki Shinji, Morimoto Mutsuko Y., Morisawa Toshiyuki, Moriwaki Shigenori, Mukohyama Shinji, Nagano Shigeo, Nakamura Kouji, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nishida Erina, Nishizawa Atsushi, Niwa Yoshito, Noumi Taiga, Obuchi Yoshiyuki, Ohishi Naoko, Ohkawa Masashi, Okada Kenshi, Okada Norio, Okutomi Koki, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Saito Ryo, Sakagami Masaaki, Sakai Shin-ichiro, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shibata Kazunori, Shimo-oku Ayumi, Shinkai Hisaaki, Shoda Ayaka, Somiya Kentaro, Sotani Hajime, Suemasa Aru, Sugiyama Naoshi, Suwa Yudai, Suzuki Rieko, Tagoshi Hideyuki, Takahashi Fuminobu, Takahashi Kakeru, Takahashi Keitaro, Takahashi Ryutaro, Takahashi Ryuichi, Takahashi Hirotaka, Akiteru Takamori, Takano Tadashi, Tanaka Nobuyuki, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Torii Yasuo, Toyoshima Morio, Tsujikawa Shinji, Ueda Akitoshi, Ueda Ken-ichi, Ushiba Takafumi, Utashima Masayoshi, Wakabayashi Yaka, Yagi Kent, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh

    INTERNATIONAL JOURNAL OF MODERN PHYSICS D   28 ( 12 )   2019.09( ISSN:0218-2718

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    DOI: 10.1142/S0218271818450013

  • Space gravitational-wave antennas DECIGO and B-DECIGO Reviewed

    Kawamura Seiji, Nakamura Takashi, Ando Masaki, Seto Naoki, Akutsu Tomotada, Funaki Ikkoh, Ioka Kunihito, Kanda Nobuyuki, Kawano Isao, Musha Mitsuru, Nakazawa Kazuhiro, Sato Shuichi, Takashima Takeshi, Tanaka Takahiro, Tsubono Kimio, Yokoyama Jun'ichi, Agatsuma Kazuhiro, Aoyanagi Koh-suke, Arai Koji, Araya Akito, Aritomi Naoki, Asada Hideki, Aso Yoichi, Chen Dan, Chiba Takeshi, Ebisuzaki Toshikazu, Eguchi Satoshi, Ejiri Yumiko, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Gondo Rina, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T, Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Izumi Kiwamu, Kanemura Shinya, Kawashima Nobuki, Kawazoe Fumiko, Kishimoto Naoko, Kiuchi Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Kuroyanagi Sachiko, Maeda Kei-ichi, Matsuhara Hideo, Matsumoto Nobuyuki, Michimura Yuta, Miyakawa Osamu, Miyamoto Umpei, Miyoki Shinji, Morimoto Mutsuko Y, Morisawa Toshiyuki, Moriwaki Shigenori, Mukohyama Shinji, Nagano Shigeo, Nakamura Kouji, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nishida Erina, Nishizawa Atsushi, Niwa Yoshito, Noumi Taiga, Obuchi Yoshiyuki, Ohishi Naoko, Ohkawa Masashi, Okada Kenshi, Okada Norio, Okutomi Koki, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Saito Ryo, Sakagami Masaaki, Sakai Shin-ichiro, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shibata Kazunori, Shimo-oku Ayumi, Shinkai Hisaaki, Shoda Ayaka, Somiya Kentaro, Sotani Hajime, Suemasa Aru, Sugiyama Naoshi, Suwa Yudai, Suzuki Rieko, Tagoshi Hideyuki, Takahashi Fuminobu, Takahashi Kakeru, Takahashi Keitaro, Takahashi Ryutaro, Takahashi Ryuichi, Takahashi Hirotaka, Akiteru Takamori, Takano Tadashi, Tanaka Nobuyuki, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Torii Yasuo, Toyoshima Morio, Tsujikawa Shinji, Ueda Akitoshi, Ueda Ken-ichi, Ushiba Takafumi, Utashima Masayoshi, Wakabayashi Yaka, Yagi Kent, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh

    INTERNATIONAL JOURNAL OF MODERN PHYSICS D   28 ( 12 )   2019.09( ISSN:0218-2718 ( eISSN:1793-6594

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    DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO) is a future Japanese space gravitational-wave antenna. The most important objective of DECIGO, among various sciences to be aimed at, is to detect gravitational waves coming from the inflation of the universe. DECIGO consists of four clusters of spacecraft, and each cluster consists of three spacecraft with three Pabry-Perot Michelson interferometers. As a pathfinder mission of DECIGO, B-DECIGO will be launched, hopefully in the 2020s, to demonstrate technologies necessary for DECIGO as well as to lead to fruitful multimessenger astronomy. B-DECIGO is a small-scale or simpler version of DECIGO with the sensitivity slightly worse than that of DECIGO, yet good enough to provide frequent detection of gravitational waves.

    DOI: 10.1142/S0218271818450013

  • First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA Reviewed

    Akutsu T., Ando M., Arai K., Arai Y., Araki S., Araya A., Aritomi N., Asada H., Aso Y., Atsuta S., Awai K., Bae S., Baiotti L., Barton M. A., Cannon K., Capocasa E., Chen C-S, Chiu T-W, Cho K., Chu Y-K, Craig K., Creus W., Doi K., Eda K., Enomoto Y., Flaminio R., Fujii Y., Fujimoto M-K, Fukunaga M., Fukushima M., Furuhata T., Hagiwara A., Haino S., Hasegawa K., Hashino K., Hayama K., Hirobayashi S., Hirose E., Hsieh B. H., Huang C-Z, Ikenoue B., Inoue Y., Ioka K., Itoh Y., Izumi K., Kaji T., Kajita T., Kakizaki M., Kamiizumi M., Kanbara S., Kanda N., Kanemura S., Kaneyama M., Kang G., Kasuya J., Kataoka Y., Kawai N., Kawamura S., Kawasaki T., Kim C., Kim J., Kim J. C., Kim W. S., Kim Y-M, Kimura N., Kinugawa T., Kirii S., Kitaoka Y., Kitazawa H., Kojima Y., Kokeyama K., Komori K., Kong A. K. H., Kotake K., Kozu R., Kumar R., Kuo H-S, Kuroyanagi S., Lee H. K., Lee H. M., Lee H. W., Leonardi M., Lin C-Y, Lin F-L, Liu G. C., Liu Y., Majorana E., Mano S., Marchio M., Matsui T., Matsushima F., Michimura Y., Mio N., Miyakawa O., Miyamoto A., Miyamoto T., Miyo K., Miyoki S., Morii W., Morisaki S., Moriwaki Y., Morozumi T., Murakami I, Musha M., Nagano K., Nagano S., Nakamura K., Nakamura T., Nakano H., Nakano M., Nakao K., Namai Y., Narikawa T., Naticchioni L., Quynh L. Nguyen, Ni W-T, Nishizawa A., Obuchi Y., Ochi T., Oh J. J., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Okutomi K., Ono K., Oohara K., Ooi C. P., Pan S-S, Park J., Arellano F. E. Pena, Pinto I, Sago N., Saijo M., Saito Y., Saitou S., Sakai K., Sakai Y., Sasai M., Sasaki M., Sasaki Y., Sato N., Sato S., Sato T., Sekiguchi Y., Seto N., Shibata M., Shimoda T., Shinkai H., Shishido T., Shoda A., Somiya K., Son E. J., Suemasa A., Suzuki T., Tagoshi H., Tahara H., Takahashi H., Takahashi R., Takamori A., Takeda H., Tanaka H., Tanaka K., Tanaka T., Tanioka S., San Martin E. N. Tapia, Tatsumi D., Terashima S., Tomaru T., Tomura T., Travasso F., Tsubono K., Tsuchida S., Uchikata N., Uchiyama T., Ueda A., Uehara T., Ueki S., Ueno K., Uraguchi F., Ushiba T., van Putten M. H. P. M., Vocca H., Wada S., Wakamatsu T., Watanabe Y., Xu W-R, Yamada T., Yamamoto A., Yamamoto K., Yamamoto S., Yamamoto T., Yokogawa K., Yokoyama J., Yokozawa T., Yoon T. H., Yoshioka T., Yuzurihara H., Zeidler S., Zhu Z-H

    CLASSICAL AND QUANTUM GRAVITY   36 ( 16 )   2019.08( ISSN:0264-9381

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    DOI: 10.1088/1361-6382/ab28a9

  • First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA Reviewed

    T Akutsu, M Ando, K Arai, Y Arai, S Araki, A Araya, N Aritomi, H Asada, Y Aso, S Atsuta, K Awai, S Bae, L Baiotti, M A Barton, K Cannon, E Capocasa, C-S Chen, T-W Chiu, K Cho, Y-K Chu, K Craig, W Creus, K Doi, K Eda, Y Enomoto, R Flaminio, Y Fujii, M-K Fujimoto, M Fukunaga, M Fukushima, T Furuhata, A Hagiwara, S Haino, K Hasegawa, K Hashino, K Hayama, S Hirobayashi, E Hirose, B H Hsieh, C-Z Huang, B Ikenoue, Y Inoue, K Ioka, Y Itoh, K Izumi, T Kaji, T Kajita, M Kakizaki, M Kamiizumi, S Kanbara, N Kanda, S Kanemura, M Kaneyama, G Kang, J Kasuya, Y Kataoka, N Kawai, S Kawamura, T Kawasaki, C Kim, J Kim, J C Kim, W S Kim, Y-M Kim, N Kimura, T Kinugawa, S Kirii, Y Kitaoka, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A K H Kong, K Kotake, R Kozu, R Kumar, H-S Kuo, S Kuroyanagi, H K Lee, H M Lee, H W Lee, M Leonardi, C-Y Lin, F-L Lin, G C Liu, Y Liu, E Majorana, S Mano, M Marchio, T Matsui, F Matsushima, Y Michimura, N Mio, O Miyakawa, A Miyamoto, T Miyamoto, K Miyo, S Miyoki, W Morii, S Morisaki, Y Moriwaki, T Morozumi, I Murakami, M Musha, K Nagano, S Nagano, K Nakamura, T Nakamura, H Nakano, M Nakano, K Nakao, Y Namai, T Narikawa, L Naticchioni, L Nguyen Quynh, W-T Ni, A Nishizawa, Y Obuchi, T Ochi, J J Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, K Okutomi, K Ono, K Oohara, C P Ooi, S-S Pan, J Park, F E Peña Arellano, I Pinto, N Sago, M Saijo, Y Saito, S Saitou, K Sakai, Y Sakai, Y Sakai, M Sasai, M Sasaki, Y Sasaki, N Sato, S Sato, T Sato, Y Sekiguchi, N Seto, M Shibata, T Shimoda, H Shinkai, T Shishido, A Shoda, K Somiya, E J Son, A Suemasa, T Suzuki, T Suzuki, H Tagoshi, H Tahara, H Takahashi, R Takahashi, A Takamori, H Takeda, H Tanaka, K Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, D Tatsumi, S Terashima, T Tomaru, T Tomura, F Travasso, K Tsubono, S Tsuchida, N Uchikata, T Uchiyama, A Ueda, T Uehara, S Ueki, K Ueno, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, S Wada, T Wakamatsu, Y Watanabe, W-R Xu, T Yamada, A Yamamoto, K Yamamoto, K Yamamoto, S Yamamoto, T Yamamoto, K Yokogawa, J Yokoyama, T Yokozawa, T H Yoon, T Yoshioka, H Yuzurihara, S Zeidler, Z-H Zhu

    Classical and Quantum Gravity   36 ( 16 )   165008 - 165008   2019.08( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/1361-6382/ab28a9

    Other URL: https://iopscience.iop.org/article/10.1088/1361-6382/ab28a9

  • Development of prototype RICH detector with multi-anode photomultipliers for radioactive ions

    Machida M.

    Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment   931   23 - 28   2019.07( ISSN:01689002

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    DOI: 10.1016/j.nima.2019.03.085

  • Vibration isolation system with a compact damping system for power recycling mirrors of KAGRA Reviewed

    Akiyama Y., Akutsu T., Ando M., Arai K., Arai Y., Araki S., Araya A., Aritomi N., Asada H., Aso Y., Bae S., Baiotti L., Barton M. A., Cannon K., Capocasa E., Chen C-S, Chiu T-W, Cho K., Chu Y-K, Craig K., Dattilo V, Doi K., Enomoto Y., Flaminio R., Fujii Y., Fujimoto M-K, Fukunaga M., Fukushima M., Furuhata T., Haino S., Hasegawa K., Hashimoto Y., Hashino K., Hayama K., Hirayama T., Hirose E., Hsieh B. H., Huang C-Z, Ikenoue B., Inoue Y., Ioka K., Itoh Y., Izumi K., Kaji T., Kajita T., Kakizaki M., Kamiizumi M., Kanbara S., Kanda N., Kanemura S., Kang G., Kasuya J., Kawai N., Kawasaki T., Kim C., Kim W. S., Kim J., Kim J. C., Kimura N., Kirii S., Kitaoka Y., Kitazawa H., Kojima Y., Kokeyama K., Komori K., Kong A., Kotake K., Kozu R., Kumar R., Kuo H-S, Kuroki S., Kuroyanagi S., Lee H. K., Lee H. M., Lee H. W., Leonardi M., Lin C-Y, Lin F-L, Liu G. C., Marchio M., Matsui T., Michimura Y., Mio N., Miyakawa O., Miyamoto A., Miyoki S., Morii W., Morisaki S., Moriwaki Y., Musha M., Nagano S., Nagano K., Nakamura K., Nakamura T., Nakano H., Nakano M., Narikawa T., Nguyen Quynh L., Ni W-T, Nishizawa A., Obuchi Y., Oh J., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Okutomi K., Ono K., Oohara K., Ooi C. P., Pan S-S, Paoletti F., Park J., Passaquieti R., Pena Arellano F. E., Sago N., Saito S., Saito Y., Sakai K., Sakai Y., Sasai M., Sato S., Sato T., Sekiguchi T., Sekiguchi Y., Shibata M., Shimoda T., Shinkai H., Shishido T., Shoda A., Someya N., Somiya K., Son E. J., Suemasa A., Suzuki T., Suzuki T., Tagoshi H., Tahara H., Takahashi H., Takahashi R., Takeda H., Tanaka H., Tanaka K., Tanaka T., Tanioka S., San Martin E. N. Tapia, Tomaru T., Tomura T., Travasso F., Tsubono K., Tsuchida S., Uchikata N., Uchiyama T., Uehara T., Ueno K., Uraguchi F., Ushiba T., Van Putten M. H. P. M., Vocca H., Wakamatsu T., Watanabe Y., Xu W-R, Yamada T., Yamamoto K., Yamamoto K., Yamamoto S., Yamamoto T., Yokogawa K., Yokoyama J., Yokozawa T., Yoshioka T., Yuzurihara H., Zeidler S., Zhu Z-H

    CLASSICAL AND QUANTUM GRAVITY   36 ( 9 )   2019.05( ISSN:0264-9381

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    DOI: 10.1088/1361-6382/ab0fcb

  • Vibration isolation system with a compact damping system for power recycling mirrors of KAGRA Reviewed

    Y Akiyama, T Akutsu, M Ando, K Arai, Y Arai, S Araki, A Araya, N Aritomi, H Asada, Y Aso, S Bae, L Baiotti, M A Barton, K Cannon, E Capocasa, C-S Chen, T-W Chiu, K Cho, Y-K Chu, K Craig, V Dattilo, K Doi, Y Enomoto, R Flaminio, Y Fujii, M-K Fujimoto, M Fukunaga, M Fukushima, T Furuhata, S Haino, K Hasegawa, Y Hashimoto, K Hashino, K Hayama, T Hirayama, E Hirose, B H Hsieh, C-Z Huang, B Ikenoue, Y Inoue, K Ioka, Y Itoh, K Izumi, T Kaji, T Kajita, M Kakizaki, M Kamiizumi, S Kanbara, N Kanda, S Kanemura, G Kang, J Kasuya, N Kawai, T Kawasaki, C Kim, W S Kim, J Kim, J C Kim, N Kimura, S Kirii, Y Kitaoka, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A Kong, K Kotake, R Kozu, R Kumar, H-S Kuo, S Kuroki, S Kuroyanagi, H K Lee, H M Lee, H W Lee, M Leonardi, C-Y Lin, F-L Lin, G C Liu, M Marchio, T Matsui, Y Michimura, N Mio, O Miyakawa, A Miyamoto, S Miyoki, W Morii, S Morisaki, Y Moriwaki, M Musha, S Nagano, K Nagano, K Nakamura, T Nakamura, H Nakano, M Nakano, T Narikawa, L Nguyen Quynh, W-T Ni, A Nishizawa, Y Obuchi, J Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, K Okutomi, K Ono, K Oohara, C P Ooi, S-S Pan, F Paoletti, J Park, R Passaquieti, F E Peña Arellano, N Sago, S Saito, Y Saito, K Sakai, Y Sakai, M Sasai, S Sato, T Sato, T Sekiguchi, Y Sekiguchi, M Shibata, T Shimoda, H Shinkai, T Shishido, A Shoda, N Someya, K Somiya, E J Son, A Suemasa, T Suzuki, T Suzuki, H Tagoshi, H Tahara, H Takahashi, R Takahashi, H Takeda, H Tanaka, K Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, T Tomaru, T Tomura, F Travasso, K Tsubono, S Tsuchida, N Uchikata, T Uchiyama, T Uehara, K Ueno, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, T Wakamatsu, Y Watanabe, W-R Xu, T Yamada, K Yamamoto, K Yamamoto, S Yamamoto, T Yamamoto, K Yokogawa, J Yokoyama, T Yokozawa, T Yoshioka, H Yuzurihara, S Zeidler, Z-H Zhu

    Classical and Quantum Gravity   36 ( 9 )   095015 - 095015   2019.05( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/1361-6382/ab0fcb

    Other URL: https://iopscience.iop.org/article/10.1088/1361-6382/ab0fcb/pdf

  • KAGRA: 2.5 generation interferometric gravitational wave detector Reviewed

    Akutsu T., Ando M., Arai K., Arai Y., Araki S., Araya A., Aritomi N., Asada H., Aso Y., Atsuta S., Awai K., Bae S., Baiotti L., Barton M. A., Cannon K., Capocasa E., Chen C-S., Chiu T-W., Cho K., Chu Y-K., Craig K., Creus W., Doi K., Eda K., Enomoto Y., Flaminio R., Fujii Y., Fujimoto M. -K., Fukunaga M., Fukushima M., Furuhata T., Haino S., Hasegawa K., Hashino K., Hayama K., Hirobayashi S., Hirose E., Hsieh B. H., Huang C-Z., Ikenoue B., Inoue Y., Ioka K., Itoh Y., Izumi K., Kaji T., Kajita T., Kakizaki M., Kamiizumi M., Kanbara S., Kanda N., Kanemura S., Kaneyama M., Kang G., Kasuya J., Kataoka Y., Kawai N., Kawamura S., Kawasaki T., Kim C., Kim J., Kim J. C., Kim W. S., Kim Y. -M., Kimura N., Kinugawa T., Kirii S., Kitaoka Y., Kitazawa H., Kojima Y., Kokeyama K., Komori K., Kong A. K. H., Kotake K., Kozu R., Kumar R., Kuo H-S., Kuroyanagi S., Lee H. K., Lee H. M., Lee H. W., Leonardi M., Lin C-Y., Lin F-L., Liu G. C., Liu Y., Majorana E., Mano S., Marchio M., Matsui T., Matsushima F., Michimura Y., Mio N., Miyakawa O., Miyamoto A., Miyamoto T., Miyo K., Miyoki S., Morii W., Morisaki S., Moriwaki Y., Morozumi T., Musha M., Nagano K., Nagano S., Nakamura K., Nakamura T., Nakano H., Nakano M., Nakao K., Narikawa T., Naticchioni L., Quynh L. Nguyen, Ni W. -T., Nishizawa A., Obuchi Y., Ochi T., Oh J. J., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Okutomi K., Ono K., Oohara K., Ooi C. P., Pan S-S., Park J., Arellano F. E. Pena, Pinto I., Sago N., Saijo M., Saitou S., Saito Y., Sakai K., Sakai Y., Sakai Y., Sasai M., Sasaki M., Sasaki Y., Sato S., Sato N., Sato T., Sekiguchi Y., Seto N., Shibata M., Shimoda T., Shinkai H., Shishido T., Shoda A., Somiya K., Son E. J., Suemasa A., Suzuki T., Suzuki T., Tagoshi H., Tahara H., Takahashi H., Takahashi R., Takamori A., Takeda H., Tanaka H., Tanaka K., Tanaka T., Tanioka S., San Martin E. N. Tapia, Tatsumi D., Tomaru T., Tomura T., Travasso F., Tsubono K., Tsuchida S., Uchikata N., Uchiyama T., Uehara T., Ueki S., Ueno K., Uraguchi F., Ushiba T., van Putten M. H. P. M., Vocca H., Wada S., Wakamatsu T., Watanabe Y., Xu W-R., Yamada T., Yamamoto A., Yamamoto K., Yamamoto K., Yamamoto S., Yamamoto T., Yokogawa K., Yokoyama J., Yokozawa T., Yoon T. H., Yoshioka T., Yuzurihara H., Zeidler S., Zhu Z. -H.

    NATURE ASTRONOMY   3 ( 1 )   35 - 40   2019.01( ISSN:2397-3366

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    DOI: 10.1038/s41550-018-0658-y

  • KAGRA: 2.5 generation interferometric gravitational wave detector Reviewed

    Akutsu T, Ando M, Arai K, Arai Y, Araki S, Araya A, Aritomi N, Asada H, Aso Y, Atsuta S, Awai K, Bae S, Baiotti L, Barton M. A, Cannon K, Capocasa E, Chen C-S, Chiu T-W, Cho K, Chu Y-K, Craig K, Creus W, Doi K, Eda K, Enomoto Y, Flaminio R, Fujii Y, Fujimoto M. -K, Fukunaga M, Fukushima M, Furuhata T, Haino S, Hasegawa K, Hashino K, Hayama K, Hirobayashi S, Hirose E, Hsieh B. H, Huang C-Z, Ikenoue B, Inoue Y, Ioka K, Itoh Y, Izumi K, Kaji T, Kajita T, Kanda N

    NATURE ASTRONOMY   3 ( 1 )   35 - 40   2019.01( ISSN:2397-3366

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    The recent detections of gravitational waves (GWs) reported by the LIGO and Virgo collaborations have made a significant impact on physics and astronomy. A global network of GW detectors will play a key role in uncovering the unknown nature of the sources in coordinated observations with astronomical telescopes and detectors. Here we introduce KAGRA, a new GW detector with two 3 km baseline arms arranged in an 'L' shape. KAGRA's design is similar to the second generations of Advanced LIGO and Advanced Virgo, but it will be operating at cryogenic temperatures with sapphire mirrors. This low-temperature feature is advantageous for improving the sensitivity around 100 Hz and is considered to be an important feature for the third-generation GW detector concept (for example, the Einstein Telescope of Europe or the Cosmic Explorer of the United States). Hence, KAGRA is often called a 2.5-generation GW detector based on laser interferometry. KAGRA's first observation run is scheduled in late 2019, aiming to join the third observation run of the advanced LIGO-Virgo network. When operating along with the existing GW detectors, KAGRA will be helpful in locating GW sources more accurately and determining the source parameters with higher precision, providing information for follow-up observations of GW trigger candidates.

    DOI: 10.1038/s41550-018-0658-y

  • Data Analysis of Gravitational Waves from the SASI mode in a core collapse supernova with the Hilbert-Huang Transform

    Takeda M., Watanabe Y., Hiranuma Y., Oohara K., Kanda N., Kuroda T., Kotake K., Sakai K., Sakai Y., Sawada T., Takahashi H., Takiwaki T., Tsuchida S., Hayama K., Yokozawa T.

    Meeting Abstracts of the Physical Society of Japan   74.2   375 - 375   2019( eISSN:2189-0803

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    DOI: 10.11316/jpsgaiyo.74.2.0_375

    CiNii Article

  • Possible confirmation of the existence of Population III stars using a third generation gravitational wave detector

    Miyamoto Akinobu, Kinugawa Tomoya, Kanda Nobuyuki

    Meeting Abstracts of the Physical Society of Japan   74.1   484 - 484   2019( eISSN:2189-0803

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    DOI: 10.11316/jpsgaiyo.74.1.0_484

    CiNii Article

  • Development of an automatic data transfer system for KAGRA and its evaluation Reviewed

    J101-B ( 9 )   818 - 827   2018.09

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  • Development of an automatic data transfer system for KAGRA and its evaluation Reviewed

    J101-B ( 9 )   818 - 827   2018.09

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  • Development of an automatic data transfer system for KAGRA and its evaluation Reviewed

    J101-B ( 9 )   818 - 827   2018.09

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    Publishing type:Research paper (scientific journal)  

  • Development of an Automatic Data Transfer System for KAGRA and Its Evaluation Reviewed

    SAKAI Kazuki, KANDA Nobuyuki, OOHARA Ken-ichi, YAMAMOTO Takahiro, MIYAKAWA Osamu, SASAKI Yukitsugu, UEKI Satoshi, TAKAHASHI Hirotaka

    J101-B ( 9 )   818 - 827   2018.09( ISSN:13444697

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    KAGRA is a 3-km interferometric gravitational wave telescope located in the Kamioka mine in Japan. In this paper, we report on the development of an automatic data transfer system between the KAGRA site and remote storage/analysis sites. From the results of evaluation and operation during iKAGRA test operation of the constructed data transfer system, we confirmed that the constructed data transfer system was satisfied both of the requirements on transferring data without missing and on transfer performance.

    DOI: 10.14923/transcomj.2017jbp3064

  • Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators Reviewed

    Inoue Yuki, Haino Sadakazu, Kanda Nobuyuki, Ogawa Yujiro, Suzuki Toshikazu, Tomaru Takayuki, Yamanmoto Takahiro, Yokozawa Takaaki

    PHYSICAL REVIEW D   98 ( 2 )   2018.07( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.98.022005

  • Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators Reviewed

    Inoue Yuki, Haino Sadakazu, Kanda Nobuyuki, Ogawa Yujiro, Suzuki Toshikazu, Tomaru Takayuki, Yamanmoto Takahiro, Yokozawa Takaaki

    PHYSICAL REVIEW D   98 ( 2 )   2018.07( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.98.022005

  • Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA Reviewed

    Abbott B. P., Abbott R., Abbott T. D., Abernathy M. R., Acernese F., Ackley K., Adams C., Adams T., Addesso P., Adhikari R. X., Adya V. B., Affeldt C., Agathos M., Agatsuma K., Aggarwal N., Aguiar O. D., Aiello L., Ain A., Ajith P., Akutsu T., Allen B., Allocca A., Altin P. A., Ananyeva A., Anderson S. B., Anderson W. G., Ando M., Appert S., Arai K., Araya A., Araya M. C., Areeda J. S., Arnaud N., Arun K. G., Asada H., Ascenzi S., Ashton G., Aso Y., Ast M., Aston S. M., Astone P., Atsuta S., Aufmuth P., Aulbert C., Avila-Alvarez A., Awai K., Babak S., Bacon P., Bader M. K. M., Baiotti L., Baker P. T., Baldaccini F., Ballardin G., Ballmer S. W., Barayoga J. C., Barclay S. E., Barish B. C., Barker D., Barone F., Barr B., Barsotti L., Barsuglia M., Barta D., Bartlett J., Barton M. A., Bartos I., Bassiri R., Basti A., Batch J. C., Baune C., Bavigadda V., Bazzan M., Becsy B., Beer C., Bejger M., Belahcene I., Belgin M., Bell A. S., Berger B. K., Bergmann G., Berry C. P. L., Bersanetti D., Bertolini A., Betzwieser J., Bhagwat S., Bhandare R., Bilenko I. A., Billingsley G., Billman C. R., Birch J., Birney R., Birnholtz O., Biscans S., Bisht A., Bitossi M., Biwer C., Bizouard M. A., Blackburn J. K., Blackman J., Blair C. D., Blair D. G., Blair R. M., Bloemen S., Bock O., Boer M., Bogaert G., Bohe A., Bondu F., Bonnand R., Boom B. A., Bork R., Boschi V., Bose S., Bouffanais Y., Bozzi A., Bradaschia C., Brady P. R., Braginsky V. B., Branchesi M., Brau J. E., Briant T., Brillet A., Brinkmann M., Brisson V., Brockill P., Broida J. E., Brooks A. F., Brown D. A., Brown D. D., Brown N. M., Brunett S., Buchanan C. C., Buikema A., Bulik T., Bulten H. J., Buonanno A., Buskulic D., Buy C., Byer R. L., Cabero M., Cadonati L., Cagnoli G., Cahillane C., Bustillo J. Calderon, Callister T. A., Calloni E., Camp J. B., Cannon K. C., Cao H., Cao J., Capano C. D., Capocasa E., Carbognani F., Caride S., Diaz J. 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J., Hagiwara A., Hall B. R., Hall E. D., Hammond G., Haney M., Hanke M. M., Hanks J., Hanna C., Hannam M. D., Hanson J., Hardwick T., Harms J., Harry G. M., Harry I. W., Hart M. J., Hartman M. T., Haster C. -J., Haughian K., Hayama K., Healy J., Heidmann A., Heintze M. C., Heitmann H., Hello P., Hemming G., Hendry M., Heng I. S., Hennig J., Henry J., Heptonstall A. W., Heurs M., Hild S., Hirose E., Hoak D., Hofman D., Holt K., Holz D. E., Hopkins P., Hough J., Houston E. A., Howell E. J., Hu Y. M., Huerta E. A., Huet D., Hughey B., Husa S., Huttner S. H., Huynh-Dinh T., Indik N., Ingram D. R., Inta R., Ioka K., Isa H. N., Isac J. -M., Isi M., Isogai T., Itoh Y., Iyer B. R., Izumi K., Jacqmin T., Jani K., Jaranowski P., Jawahar S., Jimenez-Forteza F., Johnson W. W., Jones D. I., Jones R., Jonker R. J. G., Ju L., Junker J., Kagawa T., Kajita T., Kakizaki M., Kalaghatgi C. V., Kalogera V., Kamiizumi M., Kanda N., Kandhasamy S., Kanemura S., Kaneyama M., Kang G., Kanner J. B., Karki S., Karvinen K. S., Kasprzack M., Kataoka Y., Katsavounidis E., Katzman W., Kaufer S., Kaur T., Kawabe K., Kawai N., Kawamura S., Kefelian F., Keitel D., Kelley D. B., Kennedy R., Key J. S., Khalili F. Y., Khan I., Khan S., Khan Z., Khazanov E. A., Kijbunchoo N., Kim C., Kim H., Kim J. C., Kim J., Kim W., Kim Y. -M., Kimbrell S. J., Kimura N., King E. J., King P. J., Kirchhoff R., Kissel J. S., Klein B., Kleybolte L., Klimenko S., Koch P., Koehlenbeck S. M., Kojima Y., Kokeyama K., Koley S., Komori K., Kondrashov V., Kontos A., Korobko M., Korth W. Z., Kotake K., Kowalska I., Kozak D. B., Kraemer C., Kringel V., Krishnan B., Krolak A., Kuehn G., Kumar P., Kumar Rahul, Kumar Rakesh, Kuo L., Kuroda K., Kutynia A., Kuwahara Y., Lackey B. D., Landry M., Lang R. N., Lange J., Lantz B., Lanza R. K., Lartaux-Vollard A., Lasky P. D., Laxen M., Lazzarini A., Lazzaro C., Leaci P., Leavey S., Lebigot E. O., Lee C. H., Lee H. K., Lee H. M., Lee H. W., Lee K., Lehmann J., Lenon A., Leonardi M., Leong J. R., Leroy N., Letendre N., Levin Y., Li T. G. F., Libson A., Littenberg T. B., Liu J., Lockerbie N. A., Lombardi A. L., London L. T., Lord J. E., Lorenzini M., Loriette V., Lormand M., Losurdo G., Lough J. D., Lousto C. O., Lovelace G., Lueck H., Lundgren A. P., Lynch R., Ma Y., Macfoy S., Machenschalk B., MacInnis M., Macleod D. M., Magana-Sandoval F., Majorana E., Maksimovic I., Malvezzi V., Man N., Mandic V., Mangano V., Mano S., Mansell G. L., Manske M., Mantovani M., Marchesoni F., Marchio M., Marion F., Marka S., Marka Z., Markosyan A. S., Maros E., Martelli F., Martellini L., Martin I. W., Martynov D. V., Mason K., Masserot A., Massinger T. J., Masso-Reid M., Mastrogiovanni S., Matichard F., Matone L., Matsumoto N., Matsushima F., Mavalvala N., Mazumder N., McCarthy R., McClelland D. E., McCormick S., McGrath C., McGuire S. C., McIntyre G., McIver J., McManus D. J., McRae T., McWilliams S. T., Meacher D., Meadors G. D., Meidam J., Melatos A., Mendell G., Mendoza-Gandara D., Mercer R. A., Merilh E. L., Merzougui M., Meshkov S., Messenger C., Messick C., Metzdorff R., Meyers P. M., Mezzani F., Miao H., Michel C., Michimura Y., Middleton H., Mikhailov E. E., Milano L., Miller A. L., Miller A., Miller B. B., Miller J., Millhouse M., Minenkov Y., Ming J., Mirshekari S., Mishra C., Mitrofanov V. P., Mitselmakher G., Mittleman R., Miyakawa O., Miyamoto A., Miyamoto T., Miyoki S., Moggi A., Mohan M., Mohapatra S. R. P., Montani M., Moore B. C., Moore C. J., Moraru D., Moreno G., Morii W., Morisaki S., Moriwaki Y., Morriss S. R., Mours B., Mow-Lowry C. M., Mueller G., Muir A. W., Mukherjee Arunava, Mukherjee D., Mukherjee S., Mukund N., Mullavey A., Munch J., Muniz E. A. M., Murray P. G., Mytidis A., Nagano S., Nakamura K., Nakamura T., Nakano H., Nakano Masaya, Nakano Masayuki, Nakao K., Napier K., Nardecchia I., Narikawa T., Naticchioni L., Nelemans G., Nelson T. J. N., Neri M., Nery M., Neunzert A., Newport J. M., Newton G., Nguyen T. T., Ni W. -T., Nielsen A. B., Nissanke S., Nitz A., Noack A., Nocera F., Nolting D., Normandin M. E. N., Nuttall L. K., Oberling J., Ochsner E., Oelker E., Ogin G. H., Oh J. J., Oh S. H., Ohashi M., Ohishi N., Ohkawa M., Ohme F., Okutomi K., Oliver M., Ono K., Ono Y., Oohara K., Oppermann P., Oram Richard J., O'Reilly B., O'Shaughnessy R., Ottaway D. J., Overmier H., Owen B. J., Pace A. E., Page J., Pai A., Pai S. A., Palamos J. R., Palashov O., Palomba C., Pal-Singh A., Pan H., Pankow C., Pannarale F., Pant B. C., Paoletti F., Paoli A., Papa M. A., Paris H. R., Parker W., Pascucci D., Pasqualetti A., Passaquieti R., Passuello D., Patricelli B., Pearlstone B. L., Pedraza M., Pedurand R., Pekowsky L., Pele A., Pena Arellano F. E., Penn S., Perez C. J., Perreca A., Perri L. M., Pfeiffer H. P., Phelps M., Piccinni O. J., Pichot M., Piergiovanni F., Pierro V., Pillant G., Pinard L., Pinto I. M., Pitkin M., Poe M., Poggiani R., Popolizio P., Post A., Powell J., Prasad J., Pratt J. W. W., Predoi V., Prestegard T., Prijatelj M., Principe M., Privitera S., Prodi G. A., Prokhorov L. G., Puncken O., Punturo M., Puppo P., Puerrer M., Qi H., Qin J., Qiu S., Quetschke V., Quintero E. A., Quitzow-James R., Raab F. J., Rabeling D. S., Radkins H., Raffai P., Raja S., Rajan C., Rakhmanov M., Rapagnani P., Raymond V., Razzano M., Re V., Read J., Regimbau T., Rei L., Reid S., Reitze D. H., Rew H., Reyes S. D., Rhoades E., Ricci F., Riles K., Rizzo M., Robertson N. A., Robie R., Robinet F., Rocchi A., Rolland L., Rollins J. G., Roma V. J., Romano R., Romie J. H., Rosinska D., Rowan S., Ruediger A., Ruggi P., Ryan K., Sachdev S., Sadecki T., Sadeghian L., Sago N., Saijo M., Saito Y., Sakai K., Sakellariadou M., Salconi L., Saleem M., Salemi F., Samajdar A., Sammut L., Sampson L. M., Sanchez E. J., Sandberg V., Sanders J. R., Sasaki Y., Sassolas B., Sathyaprakash B. S., Sato S., Sato T., Saulson P. R., Sauter O., Savage R. L., Sawadsky A., Schale P., Scheuer J., Schmidt E., Schmidt J., Schmidt P., Schnabel R., Schofield R. M. S., Schoenbeck A., Schreiber E., Schuette D., Schutz B. F., Schwalbe S. G., Scott J., Scott S. M., Sekiguchi T., Sekiguchi Y., Sellers D., Sengupta A. S., Sentenac D., Sequino V., Sergeev A., Setyawati Y., Shaddock D. A., Shaffer T. J., Shahriar M. S., Shapiro B., Shawhan P., Sheperd A., Shibata M., Shikano Y., Shimoda T., Shoda A., Shoemaker D. H., Shoemaker D. M., Siellez K., Siemens X., Sieniawska M., Sigg D., Silva A. D., Singer A., Singer L. P., Singh A., Singh R., Singhal A., Sintes A. M., Slagmolen B. J. J., Smith B., Smith J. R., Smith R. J. E., Somiya K., Son E. J., Sorazu B., Sorrentino F., Souradeep T., Spencer A. P., Srivastava A. K., Staley A., Steinke M., Steinlechner J., Steinlechner S., Steinmeyer D., Stephens B. C., Stevenson S. P., Stone R., Strain K. A., Straniero N., Stratta G., Strigin S. E., Sturani R., Stuver A. L., Sugimoto Y., Summerscales T. Z., Sun L., Sunil S., Sutton P. J., Suzuki T., Swinkels B. L., Szczepanczyk M. J., Tacca M., Tagoshi H., Takada S., Takahashi H., Takahashi R., Takamori A., Talukder D., Tanaka H., Tanaka K., Tanaka T., Tanner D. B., Tapai M., Taracchini A., Tatsumi D., Taylor R., Telada S., Theeg T., Thomas E. G., Thomas M., Thomas P., Thorne K. A., Thrane E., Tippens T., Tiwari S., Tiwari V., Tokmakov K. V., Toland K., Tomaru T., Tomlinson C., Tonelli M., Tornasi Z., Torrie C. I., Toeyrae D., Travasso F., Traylor G., Trifiro D., Trinastic J., Tringali M. C., Trozzo L., Tse M., Tso R., Tsubono K., Tsuzuki T., Turconi M., Tuyenbayev D., Uchiyama T., Uehara T., Ueki S., Ueno K., Ugolini D., Unnikrishnan C. S., Urban A. L., Ushiba T., Usman S. A., Vahlbruch H., Vajente G., Valdes G., van Bakel N., van Beuzekom M., van den Brand J. F. J., Van Den Broeck C., Vander-Hyde D. C., van der Schaaf L., van Heijningen J. V., van Putten M. H. P. M., van Veggel A. A., Vardaro M., Varma V., Vass S., Vasuth M., Vecchio A., Vedovato G., Veitch J., Veitch P. J., Venkateswara K., Venugopalan G., Verkindt D., Vetrano F., Vicere A., Viets A. D., Vinciguerra S., Vine D. J., Vinet J. -Y., Vitale S., Vo T., Vocca H., Vorvick C., Voss D. V., Vousden W. D., Vyatchanin S. P., Wade A. R., E. L., Wade M., Wakamatsu T., Walker M., Wallace L., Walsh S., Wang G., Wang H., Wang M., Wang Y., Ward R. L., Warner J., Was M., Watchi J., Weaver B., Wei L. -W., Weinert M., Weinstein A. J., Weiss R., Wen L., Wessels P., Westphal T., Wette K., Whelan J. T., Whiting B. F., Whittle C., Williams D., Williams R. D., Williamson A. R., Willis J. L., Willke B., Wimmer M. H., Winkler W., Wipf C. C., Wittel H., Woan G., Woehler J., Worden J., Wright J. L., Wu D. S., Wu G., Yam W., Yamamoto H., Yamamoto K., Yamamoto T., Yancey C. C., Yano K., Yap M. J., Yokoyama J., Yokozawa T., Yoon T. H., Yu Hang, Yu Haocun, Yuzurihara H., Yvert M., Zadrozny A., Zangrando L., Zanolin M., Zeidler S., Zendri J. -P., Zevin M., Zhang L., Zhang M., Zhang T., Zhang Y., Zhao C., Zhou M., Zhou Z., Zhu S. J., Zhu X. J., Zucker M. E., Zweizig J.

    LIVING REVIEWS IN RELATIVITY   21   2018.04

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    DOI: 10.1007/s41114-018-0012-9

  • Construction of KAGRA: an underground gravitational-wave observatory Reviewed

    Akutsu T., Ando M., Araki S., Araya A., Arima T., Aritomi N., Asada H., Aso Y., Atsuta S., Awai K., Baiotti L., Barton M. A., Chen D., Cho K., Craig K., DeSalvo R., Doi K., Eda K., Enomoto Y., Flaminio R., Fujibayashi S., Fujii Y., Fujimoto M. -K., Fukushima M., Furuhata T., Hagiwara A., Haino S., Harita S., Hasegawa K., Hasegawa M., Hashino K., Hayama K., Hirata N., Hirose E., Ikenoue B., Inoue Y., Ioka K., Ishizaki H., Itoh Y., Jia D., Kagawa T., Kaji T., Kajita T., Kakizaki M., Kakuhata H., Kamiizumi M., Kanbara S., Kanda N., Kanemura S., Kaneyama M., Kasuya J., Kataoka Y., Kawaguchi K., Kawai N., Kawamura S., Kawazoe F., Kim C., Kim J., Kim J. C., Kim W., Kimura N., Kitaoka Y., Kobayashi K., Kojima Y., Kokeyama K., Komori K., Kotake K., Kubo K., Kumar R., Kume T., Kuroda K., Kuwahara Y., Lee H. -K., Lee H. -W., Lin C. -Y., Liu Y., Majorana E., Mano S., Marchio M., Matsui T., Matsumoto N., Matsushima F., Michimura Y., Mio N., Miyakawa O., Miyake K., Miyamoto A., Miyamoto T., Miyo K., Miyoki S., Morii W., Morisaki S., Moriwaki Y., Muraki Y., Murakoshi M., Musha M., Nagano K., Nagano S., Nakamura K., Nakamura T., Nakano H., Nakano M., Nakano M., Nakao H., Nakao K., Narikawa T., Ni W. -T., Nonomura T., Obuchi Y., Oh J. J., Oh S. -H., Ohashi M., Ohishi N., Ohkawa M., Ohmae N., Okino K., Okutomi K., Ono K., Ono Y., Oohara K., Ota S., Park J., Pena Arellano F. E., Pinto I. M., Principe M., Sago N., Saijo M., Saito T., Saito Y., Saitou S., Sakai K., Sakakibara Y., Sasaki Y., Sato S., Sato T., Sato Y., Sekiguchi T., Sekiguchi Y., Shibata M., Shiga K., Shikano Y., Shimoda T., Shinkai H., Shoda A., Someya N., Somiya K., Son E. J., Starecki T., Suemasa A., Sugimoto Y., Susa Y., Suwabe H., Suzuki T., Tachibana Y., Tagoshi H., Takada S., Takahashi H., Takahashi R., Takamori A., Takeda H., Tanaka H., Tanaka K., Tanaka T., Tatsumi D., Telada S., Tomaru T., Tsubono K., Tsuchida S., Tsukada L., Tsuzuki T., Uchikata N., Uchiyama T., Uehara T., Ueki S., Ueno K., Uraguchi F., Ushiba T., van Putten M. H. P. M., Wada S., Wakamatsu T., Yaginuma T., Yamamoto K., Yamamoto S., Yamamoto T., Yano K., Yokoyama J., Yokozawa T., Yoon T. H., Yuzurihara H., Zeidler S., Zhao Y., Zheng L., Agatsuma K., Akiyama Y., Arai N., Asano M., Bertolini A., Fujisawa M., Goetz R., Guscott J., Hashimoto Y., Hayashida Y., Hennes E., Hirai K., Hirayama T., Ishitsuka H., Kato J., Khalaidovski A., Koike S., Kumeta A., Miener T., Morioka M., Mueller C. L., Narita T., Oda Y., Ogawa T., Sekiguchi T., Tamura H., Tanner D. B., Tokoku C., Toritani M., Utsuki T., Uyeshima M., van den Brand J. F. J., van Heijningen J. V., Yamaguchi S., Yanagida A.

    PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS   ( 1 )   2018.01( ISSN:2050-3911

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1093/ptep/ptx180

  • Construction of KAGRA: an underground gravitational-wave observatory Reviewed

    KAGRA Collaboration, Shoda, A, Ikenoue, B, Tatsumi, D, Uraguchi, F, Peña Arellano, F E, Ishizaki, H, Nakamura, K, Fukushima, M, Marchio, M, Barton, M A, Fujimoto, M -K, Hirata, N, Flaminio, R, Takahashi, R, Saitou, S, Zeidler, S, Akutsu, T, Tsuzuki, T, Aso, Y, Fujii, Y, Obuchi, Y, Ohishi, N, Ando, M, Baiotti, L, Park, J, Cho, K, Pinto, I M, Principe, M, DeSalvo, R, Matsushima, F, Tamura, H, Hashino, K, Kobayashi, K, Fujisawa, M, Kakizaki, M, Kanbara, S, Kanemura, S, Furuhata, T, Kagawa, T, Matsui, T, Moriwaki, Y, Sugimoto, Y, Nakano, H, Fujibayashi, S, Nakamura, T, Tanaka, T, Haino, S, Inoue, Y, Jia, D, Kakuhata, H, Miyake, K, Hasegawa, M, Nakano, M, Ioka, K, Kawaguchi, K, Shibata, M, Itoh, Y, Eda, K, Tsukada, L, Morisaki, S, Yokoyama, J, Kawazoe, F, Miener, T, Kim, C, Kim, J, Lee, H -W, Kim, J C, Son, E J, Oh, J J, Oh, S -H, Kim, W, Kojima, Y, Kotake, K, Kubo, K, Murakoshi, M, Someya, N, Ota, S, Nonomura, T, Sato, S, Lee, H -K, Takeda, H, Komori, K, Tsubono, K, Aritomi, N, Wada, S, Shimoda, T, Ushiba, T, Kuwahara, Y, Michimura, Y, Lin, C -Y, Majorana, E, Mano, S, Matsumoto, N, Mio, N, Ohmae, N, Morii, W, Suemasa, A, Musha, M, Nagano, S, Ni, W -T, Hagiwara, A, Kumar, R, Araki, S, Koike, S, Kume, T, Sato, Y, Kimura, N, Suzuki, T, Tomaru, T, Suwabe, H, Hirai, K, Oohara, K, Shiga, K, Ohkawa, M, Narita, T, Saito, T, Sato, T, Wakamatsu, T, Okino, K, Okutomi, K, Ono, Y, Sago, N, Saijo, M, Sakai, K, Takahashi, H, Ueki, S, Sasaki, Y, Sekiguchi, Y, Araya, A, Takamori, A, Uyeshima, M, Ogawa, T, Shikano, Y, Shinkai, H, Yamamoto, S, Starecki, T, Takada, S, Telada, S, Uehara, T, Mueller, C. L, Tanner, D B, Goetz, R, Ueno, K, van Putten, M H P M, Miyamoto, A, Nakao, H, Tagoshi, H, Yuzurihara, H, Nakao, K, Tanaka, K, Asano, M, Kaneyama, M, Toritani, M, K, a, N, Uchikata, N, Tsuchida, S, Arima, T, Kaji, T, Narikawa, T, Yokozawa, T, Kitaoka, Y, Yoon, T. H, Zhao, Y, Zheng, L, Bertolini, A, Hennes, E, van den Br, , J F J, van Heijningen, J V, Agatsuma, K, Yanagida, A, Arai, N, Hirayama, T, Sekiguchi, T, Utsuki, T, Akiyama, Y, Hashimoto, Y, Guscott, J, Morioka, M, Hayashida, Y, Yamaguchi, S, Oda, Y, Asada, H, Tokoku, C, Kumeta, A, Kasuya, J, Kato, J, Yano, K, Kawai, N, Atsuta, S, Harita, S, Yaginuma, T, Kataoka, Y, Muraki, Y, Susa, Y, Tachibana, Y, Somiya, K, Chen, D, Craig, K, Hasegawa, K, Kuroda, K, Miyo, K, Nagano, K, Ono, K, Enomoto, Y, Liu, Y, Sakakibara, Y, Hirose, E, Ishitsuka, H, Tanaka, H, Awai, K, Hayama, K, Kokeyama, K, Yamamoto, K, Kamiizumi, M, Nakano, M, Ohashi, M, Miyakawa, O, Kawamura, S, Miyoki, S, Kajita, T, Miyamoto, T, Sekiguchi, T, Uchiyama, T, Yamamoto, T, Saito, Y, Doi, K, Khalaidovski, A

    Progress of Theoretical and Experimental Physics   2018 ( 1 )   2018.01( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptx180

  • J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817 Reviewed

    Yousuke Utsumi, Masaomi Tanaka, Nozomu Tominaga, Michitoshi Yoshida, Sudhanshu Barway, Takahiro Nagayama, Tetsuya Zenko, Kentaro Aoki, Takuya Fujiyoshi, Hisanori Furusawa, Koji S. Kawabata, Shintaro Koshida, Chien-Hsiu Lee, Tomoki Morokuma, Kentaro Motohara, Fumiaki Nakata, Ryou Ohsawa, Kouji Ohta, Hirofumi Okita, Akito Tajitsu, Ichi Tanaka, Tsuyoshi Terai, Naoki Yasuda, Fumio Abe, Yuichiro Asakura, Ian A. Bond, Shota Miyazaki, Takahiro Sumi, Paul J. Tristram, Satoshi Honda, Ryosuke Itoh, Yoichi Itoh, Miho Kawabata, Kumiko Morihana, Hiroki Nagashima, Tatsuya Nakaoka, Tomohito Ohshima, Jun Takahashi, Masaki Takayama, Wako Aoki, Stefan Baar, Mamoru Doi, Francois Finet, Nobuyuki Kanda, Nobuyuki Kawai, Ji Hoon Kim, Daisuke Kuroda, Wei Liu, Kazuya Matsubayashi, Katsuhiro L. Murata, Hiroshi Nagai, Tomoki Saito, Yoshihiko Saito, Shigeyuki Sako, Yuichiro Sekiguchi, Yoichi Tamura, Masayuki Tanaka, Makoto Uemura, Masaki S. Yamaguchi

    Publications of the Astronomical Society of Japan   69 ( 6 )   101   2017.12( ISSN:0004-6264 ( eISSN:2053-051X

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    DOI: 10.1093/pasj/psx118

  • J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817 Reviewed

    Utsumi Yousuke, Tanaka Masaomi, Tominaga Nozomu, Yoshida Michitoshi, Barway Sudhanshu, Nagayama Takahiro, Zenko Tetsuya, Aoki Kentaro, Fujiyoshi Takuya, Furusawa Hisanori, Kawabata Koji S., Koshida Shintaro, Lee Chien-Hsiu, Morokuma Tomoki, Motohara Kentaro, Nakata Fumiaki, Ohsawa Ryou, Ohta Kouji, Okita Hirofumi, Tajitsu Akito, Tanaka Ichi, Terai Tsuyoshi, Yasuda Naoki, Abe Fumio, Asakura Yuichiro, Bond Ian A., Miyazaki Shota, Sumi Takahiro, Tristram Paul J., Honda Satoshi, Itoh Ryosuke, Itoh Yoichi, Kawabata Miho, Morihana Kumiko, Nagashima Hiroki, Nakaoka Tatsuya, Ohshima Tomohito, Takahashi Jun, Takayama Masaki, Aoki Wako, Baar Stefan, Doi Mamoru, Finet Francois, Kanda Nobuyuki, Kawai Nobuyuki, Kim Ji Hoon, Kuroda Daisuke, Liu Wei, Matsubayashi Kazuya, Murata Katsuhiro L., Nagai Hiroshi, Saito Tomoki, Saito Yoshihiko, Sako Shigeyuki, Sekiguchi Yuichiro, Tamura Yoichi, Tanaka Masayuki, Uemura Makoto, Yamaguchi Masaki S.

    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN   69 ( 6 )   2017.12( ISSN:0004-6264

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    DOI: 10.1093/pasj/psx118

  • Development of KAGRA Algorithmic Library (KAGALI)

    Ken’ichi Oohara, Koh Ueno, Hirotaka Yuzurihara, Yosuke Itoh, Hirotaka Takahasi, Tsukasa Arima, Kazunari Eda, Yoshinori Fujii, Kazuhiro Hayama, Yuta Hiranuma, Shigeki Hirobayashi, Nobuyuki Kanda, Masato Kaneyama, Jeongcho Kim, Chunglee Kim, Hyung Won Lee, Shuhei Mano, Kyohei Miyake, Akinobu Miyamoto, Yuta Nakanishi, Naoko Ohishi, Masaya Nakano, Hayato Nakao, Tatsuya Narikawa, Kazuki Sakai, Yukitsugu Sasaki, Ayaka Shoda, Hiroto Suwabe, Hideyuki Tagoshi, Kazuyuki Tanaka, Satoshi Ueki, Takeshi Wakamatsu, Takahiro Yamamoto, Jun’ichi Yokoyama, Takaaki Yokozawa

    The Fourteenth Marcel Grossmann Meeting   2017.12

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    Publishing type:Research paper (international conference proceedings)  

    DOI: 10.1142/9789813226609_0404

  • Multi-messenger Observations of a Binary Neutron Star Merger Reviewed International coauthorship

    Abbott B. P., et.al. (3614 persons)

    ASTROPHYSICAL JOURNAL LETTERS   848 ( 2 )   2017.10( ISSN:2041-8205

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    Publishing type:Research paper (scientific journal)   Kind of work:Joint Work  

    DOI: 10.3847/2041-8213/aa91c9

  • How to confirm the existence of population III stars by observations of gravitational waves Reviewed

    Miyamoto Akinobu, Kinugawa Tomoya, Nakamura Takashi, Kanda Nobuyuki

    PHYSICAL REVIEW D   96 ( 6 )   2017.09( ISSN:2470-0010

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.96.064025

  • How to confirm the existence of population III stars by observations of gravitational waves Reviewed

    Akinobu Miyamoto, Tomoya Kinugawa, Takashi Nakamura, Nobuyuki Kanda

    Physical Review D   96 ( 6 )   2017.09( ISSN:2470-0029

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    We propose a method for confirmation of the existence of Population III (Pop III) stars with massive black hole binaries as GW150914 in gravitational wave (GW) observation. When we get enough number of events, we want to determine which model is closer to reality, with and without Pop III stars. We need to prepare various "Pop I/II models" and various "Pop I/II/III models" and investigate which model is consistent with the events. To demonstrate our analysis, we simulate detections of GW events for some examples of population synthesis models with and without Pop III stars. We calculate the likelihood ratio with the realistic number of events and evaluate the probability of identifying the existence of Pop III stars. In typical cases, our analysis can distinguish between Pop I/II model and Pop I/II/III model with 90% probability by 22 GW signals from black hole-black hole binary mergers.

    DOI: 10.1103/PhysRevD.96.064025

  • The status of DECIGO

    Shuichi Sato, Seiji Kawamura, Masaki Ando, Takashi Nakamura, Kimio Tsubono, Akito Araya, Ikkoh Funaki, Kunihito Ioka, Nobuyuki Kanda, Shigenori Moriwaki, Mitsuru Musha, Kazuhiro Nakazawa, Kenji Numata, Shin Ichiro Sakai, Naoki Seto, Takeshi Takashima, Takahiro Tanaka, Kazuhiro Agatsuma, Koh Suke Aoyanagi, Koji Arai, Hideki Asada, Yoichi Aso, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Katsuhiko Ganzu, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki T. Inoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Nobuki Kawashima, Fumiko Kawazoe, Naoko Kishimoto, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hideaki Kudoh, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Kei Ichi Maeda, Hideo Matsuhara, Yasushi Mino, Osamu Miyakawa, Shinji Miyoki, Mutsuko Y. Morimoto, Tomoko Morioka, Toshiyuki Morisawa, Shinji Mukohyama, Shigeo Nagano, Isao Naito, Kouji Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Masashi Ohkawa, Norio Okada, Kouji Onozato, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Masaaki Sakagami, Shihori Sakata, Misao Sasaki

    Journal of Physics: Conference Series   840 ( 1 )   2017.06( ISSN:1742-6588

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    DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consists of three drag-free spacecraft arranged in an equilateral triangle with 1000 km arm lengths whose relative displacements are measured by a differential Fabry-Perot interferometer, and four units of triangular Fabry-Perot interferometers are arranged on heliocentric orbit around the sun. DECIGO is vary ambitious mission, we plan to launch DECIGO in era of 2030s after precursor satellite mission, B-DECIGO. B-DECIGO is essentially smaller version of DECIGO: B-DECIGO consists of three spacecraft arranged in an triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be late 2020s for the present..

    DOI: 10.1088/1742-6596/840/1/012010

  • The status of DECIGO

    Shuichi Sato, Seiji Kawamura, Masaki Ando, Takashi Nakamura, Kimio Tsubono, Akito Araya, Ikkoh Funaki, Kunihito Ioka, Nobuyuki Kanda, Shigenori Moriwaki, Mitsuru Musha, Kazuhiro Nakazawa, Kenji Numata, Shin Ichiro Sakai, Naoki Seto, Takeshi Takashima, Takahiro Tanaka, Kazuhiro Agatsuma, Koh Suke Aoyanagi, Koji Arai, Hideki Asada, Yoichi Aso, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Katsuhiko Ganzu, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki T. Inoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Nobuki Kawashima, Fumiko Kawazoe, Naoko Kishimoto, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hideaki Kudoh, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Kei Ichi Maeda, Hideo Matsuhara, Yasushi Mino, Osamu Miyakawa, Shinji Miyoki, Mutsuko Y. Morimoto, Tomoko Morioka, Toshiyuki Morisawa, Shinji Mukohyama, Shigeo Nagano, Isao Naito, Kouji Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Masashi Ohkawa, Norio Okada, Kouji Onozato, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Masaaki Sakagami, Shihori Sakata, Misao Sasaki

    Journal of Physics: Conference Series   840 ( 1 )   2017.06( ISSN:1742-6588 ( eISSN:1742-6596

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    DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consists of three drag-free spacecraft arranged in an equilateral triangle with 1000 km arm lengths whose relative displacements are measured by a differential Fabry-Perot interferometer, and four units of triangular Fabry-Perot interferometers are arranged on heliocentric orbit around the sun. DECIGO is vary ambitious mission, we plan to launch DECIGO in era of 2030s after precursor satellite mission, B-DECIGO. B-DECIGO is essentially smaller version of DECIGO: B-DECIGO consists of three spacecraft arranged in an triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be late 2020s for the present..

    DOI: 10.1088/1742-6596/840/1/012010

  • Gravitational Waves from Merging Intermediate-mass Black Holes. II. Event Rates at Ground-based Detectors Reviewed

    Shinkai Hisa-aki, Kanda Nobuyuki, Ebisuzaki Toshikazu

    ASTROPHYSICAL JOURNAL   835 ( 2 )   2017.02( ISSN:0004-637X

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    DOI: 10.3847/1538-4357/835/2/276

  • Gravitational Waves from Merging Intermediate-mass Black Holes. II. Event Rates at Ground-based Detectors Reviewed

    Hisa-Aki Shinkai, Nobuyuki Kanda, Toshikazu Ebisuzaki

    Astrophysical Journal   835 ( 2 )   2017.02( ISSN:1538-4357

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    Based on a dynamical formation model of a supermassive black hole (SMBH), we estimate the expected observational profile of gravitational waves at ground-based detectors, such as KAGRA or advanced LIGO/VIRGO. Noting that the second generation of detectors have enough sensitivity from 10 Hz and up (especially with KAGRA owing to its location at less seismic noise), we are able to detect the ring-down gravitational wave of a BH with mass . This enables us to check the sequence of BH mergers to SMBHs via intermediate-mass BHs. We estimate the number density of galaxies from the halo formation model and estimate the number of BH mergers from the giant molecular cloud model assuming hierarchical growth of merged cores. At the designed KAGRA (and/or advanced LIGO/VIRGO), we find that the BH merger of its total mass is at the peak of the expected mass distribution. With its signal-to-noise ratio , we estimate the event rate per year in the most optimistic case, and we also find that BH mergers in the range are per year for . Thus, if we observe a BH with more than in future gravitational-wave observations, our model naturally explains its source.

    DOI: 10.3847/1538-4357/835/2/276

  • Multi-messenger observations of a binary neutron star merger Reviewed

    B. P. Abbott, R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. X. Adhikari, V. B. Adya, C. Affeldt, M. Afrough, B. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, B. Allen, G. Allen, A. Allocca, P. A. Altin, A. Amato, A. Ananyeva, S. B. Anderson, W. G. Anderson, S. V. Angelova, S. Antier, S. Appert, K. Arai, M. C. Araya, J. S. Areeda, N. Arnaud, K. G. Arun, S. Ascenzi, G. Ashton, M. Ast, S. M. Aston, P. Astone, D. V. Atallah, P. Aufmuth, C. Aulbert, K. AultONeal, C. Austin, A. Avila-Alvarez, S. Babak, P. Bacon, M. K.M. Bader, S. Bae, P. T. Baker, F. Baldaccini, G. Ballardin, S. W. Ballmer, S. Banagiri, J. C. Barayoga, S. E. Barclay, B. C. Barish, D. Barker, K. Barkett, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, S. D. Barthelmy, J. Bartlett, I. Bartos, R. Bassiri, A. Basti, J. C. Batch, M. Bawaj, J. C. Bayley, M. Bazzan, B. Bécsy, C. Beer, M. Bejger, I. Belahcene, A. S. Bell, B. K. Berger, G. Bergmann, J. J. Bero, C. P.L. Berry, D. Bersanetti, A. Bertolini, J. Betzwieser, S. Bhagwat, R. Bhandare, I. A. Bilenko, G. Billingsley, C. R. Billman, J. Birch, R. Birney, O. Birnholtz, S. Biscans, S. Biscoveanu, A. Bisht, M. Bitossi, C. Biwer

    Astrophysical Journal Letters   848 ( 2 )   2017.01( ISSN:2041-8205 ( eISSN:2041-8213

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    © 2017. The American Astronomical Society. All rights reserved. On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40 8 8-+ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 M. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.

    DOI: 10.3847/2041-8213/aa91c9

  • Pre-DECIGO can get the smoking gun to decide the astrophysical or cosmological origin of GW150914-like binary black holes (vol 2016, 093e01, 2016) Reviewed

    Nakamura Takashi, Ando Masaki, Kinugawa Tomoya, Nakano Hiroyuki, Eda Kazunari, Sato Shuichi, Musha Mitsuru, Akutsu Tomotada, Tanaka Takahiro, Seto Naoki, Kanda Nobuyuki, Itoh Yousuke

    PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS   ( 12 )   2016.12( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptw170

  • Pre-DECIGO can get the smoking gun to decide the astrophysical or cosmological origin of GW150914-like binary black holes Reviewed

    Nakamura Takashi, Ando Masaki, Kinugawa Tomoya, Nakano Hiroyuki, Eda Kazunari, Sato Shuichi, Musha Mitsuru, Akutsu Tomotada, Tanaka Takahiro, Seto Naoki, Kanda Nobuyuki, Itoh Yousuke

    PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS   ( 9 )   2016.09( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptw127

  • Pre-DECIGO can get the smoking gun to decide the astrophysical or cosmological origin of GW150914-like binary black holes Reviewed

    Takashi Nakamura, Masaki Ando, Tomoya Kinugawa, Hiroyuki Nakano, Kazunari Eda, Shuichi Sato, Mitsuru Musha, Tomotada Akutsu, Takahiro Tanaka, Naoki Seto, Nobuyuki Kanda, Yousuke Itoh

    Prog. Theor. Exp. Phys.   2016 ( 12 )   093E01   2016.09( ISSN:2050-3911

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    DOI: 10.1093/ptep/ptw127

  • Unveiling linearly and nonlinearly correlated signals between gravitational wave detectors and environmental monitors Reviewed

    Yuzurihara Hirotaka, Hayama Kazuhiro, Mano Shuhei, Verkindt Didier, Kanda Nobuyuki

    PHYSICAL REVIEW D   94 ( 4 )   2016.08( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.94.042004

  • Unveiling linearly and nonlinearly correlated signals between gravitational wave detectors and environmental monitors Reviewed

    Hirotaka Yuzurihara, Kazuhiro Hayama, Shuhei Mano, Didier Verkindt, Nobuyuki Kanda

    Physical Review D   94 ( 4 )   2016.08( ISSN:2470-0029

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    Noise hunting is a critical requirement for realizing design sensitivity of a detector, and consequently, noise origins and its features have been revealed partially. Among the noise sources to be hunted, sources of nonlinearly correlated noise, such up-conversion noise, are hard to find and can limit the sensitivity of gravitational wave searches with advanced detectors. We propose using a correlation analysis method called maximal information coefficient (MIC) to find both nonlinear and linear correlations. We apply MIC to the scattered light noise correlated between the seismic activity and the strain signal, which limited the sensitivity of the Virgo detector during the first science run. The results show that MIC can find nonlinearly correlated noise more efficiently than the Pearson correlation method. When the data is linearly correlated, the efficiency of the Pearson method and MIC is comparable. On the other hand, when the data is known to be nonlinearly correlated, MIC finds the correlation while the Pearson method fails completely.

    DOI: 10.1103/PhysRevD.94.042004

  • Characterization of non-Gaussianity in gravitational wave detector noise Reviewed

    Yamamoto Takahiro, Hayama Kazuhiro, Mano Shuhei, Itoh Yousuke, Kanda Nobuyuki

    PHYSICAL REVIEW D   93 ( 8 )   2016.04( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.93.082005

  • The detection rate of inspiral and quasi-normal modes of Population III binary black holes which can confirm or refute the general relativity in the strong gravity region Reviewed

    Kinugawa Tomoya, Miyamoto Akinobu, Kanda Nobuyuki, Nakamura Takashi

    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY   456 ( 1 )   1093 - 1114   2016.02( ISSN:0035-8711

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    DOI: 10.1093/mnras/stv2624

  • 22aAZ-3 Digital control system for the gravitational-wave detector, KAGRA (VIII) Reviewed

    Kokeyama K., Yamamoto T., Yuzurihara H., Miyakawa O., Kamiizumi M., Awai K., Miyoki S., Michimura Y., Hayama K., Yokozawa T., Kanda N.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   71 ( 0 )   2016

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    DOI: 10.11316/jpsgaiyo.71.1.0_537

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  • 21pCD-2 iWF-MAXI : Large-Sky Soft X-Ray Transient Monitor

    Kawai N., Yatsu Y., Arimoto M., Tomida H., Ueno S., Mihara T., Serino M., Yoshida A., Sakamoto T., Tsunemi H., Kohmura T., Negoro H., Ueda Y., Tsuboi Y., Ebisawa K., Morii M., Anabuki N., Yuasa T., Dotani T., Nakamura T., Tanaka T., Yoshida Y., Kanda N., Vagins Mark

    Meeting Abstracts of the Physical Society of Japan   71   503 - 503   2016( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.71.1.0_503

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  • 初観測された重力波が開いた宇宙への新しい窓

    神田 展行

    パリティ   10月号   14 - 18   2016

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  • The detection rate of inspiral and quasi-normal modes of Population III binary black holes which can confirm or refute the general relativity in the strong gravity region Reviewed

    Tomoya Kinugawa, Akinobu Miyamoto, Nobuyuki Kanda, Takashi Nakamura

    Monthly Notices of the Royal Astronomical Society   456 ( 1 )   1093 - 1114   2016( ISSN:1365-2966

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    Using our population synthesis code, we found that the typical chirp mass defined by (m1m2)3/5/(m1 + m2)1/5 of Population III (Pop III) binary black holes (BH-BHs) is ~30M⊙ with the total mass of ~60M⊙ so that the inspiral chirp signal as well as quasi-normal mode (QNM) of the merging black hole (BH) are interesting targets of KAGRA. The detection rate of the coalescing Pop III BH-BHs is ~180 events yr-1 (SFRp/(10-2.5M⊙ yr-1 Mpc-3))([fb/(1 + fb)]/0.33)Errsys in our standard model, where SFRp, fb and Errsys are the peak value of the Pop III star formation rate, the binary fraction and the systematic error with Errsys = 1 for our standard model, respectively. To evaluate the robustness of chirp mass distribution and the range of Errsys, we examine the dependence of the results on the unknown parameters and the distribution functions in the population synthesis code. We found that the chirp mass has a peak at ~30M⊙ in most of parameters and distribution functions as well as Errsys ranges from 0.046 to 4. Therefore, the detection rate of the coalescing Pop III BH- BHs ranges about 8.3-720 events yr-1(SFRp/(10-2.5M⊙ yr-1 Mpc-3))([fb/(1 + fb)]/0.33). The minimum rate corresponds to the worst model which we think unlikely so that unless (SFRp/(10-2.5M⊙ yr-1 Mpc-3))([fb/(1 + fb)]/0.33) ⋘ 0.1, we expect the Pop III BH-BHs merger rate of at least one event per year by KAGRA. Nakano, Tanaka &amp
    Nakamura show that if signal-to-noise ratio (S/N) of QNM is larger than 35, we can confirm or refute the general relativity (GR) more than 5σ level. In our standard model, the detection rate of Pop III BH- BHs whose S/N is larger than 35 is 3.2 events yr-1 (SFRp/(10-2.5M⊙ yr-1 Mpc-3))([fb/(1 + fb)]/0.33)Errsys. Thus, there is a good chance to check whether GR is correct or not in the strong gravity region.

    DOI: 10.1093/mnras/stv2624

  • Measurement of Schumann Resonance at Kamioka Reviewed

    S. Atsuta, T. Ogawa, S. Yamaguchi, K. Hayama, A. Araya, N. Kanda, O. Miyakawa, S. Miyoki, A. Nishizawa, K. Ono, Y. Saito, K. Somiya, T. Uchiyama, M. Uyeshima, K. Yano

    11TH EDOARDO AMALDI CONFERENCE ON GRAVITATIONAL WAVES (AMALDI 11)   716   2016( ISSN:1742-6588

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    On the stochastic gravitational-wave search, correlated noise in two or more gravitational-wave detectors can be a serious problem. Schumann resonance is the name of a standing wave of electromagnetic fields, which is one of the correlated noise sources for the second-generation gravitational-wave detectors. We measured the noise levels of the environmental magnetic field both inside and outside the mine of KAGRA site at Kamioka. In this letter, we report the result of the measurement and compare the amplitude of magnetic fields inside and outside the mine to find possible issues or gain of constructing a detector underground.

    DOI: 10.1088/1742-6596/716/1/012020

  • Characterization of non-Gaussianity in gravitational wave detector noise Reviewed

    Takahiro Yamamoto, Kazuhiro Hayama, Shuhei Mano, Yousuke Itoh, Nobuyuki Kanda

    Physical Review D   93 ( 8 )   082005   2016( ISSN:2470-0010 ( eISSN:2470-0029

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    DOI: 10.1103/PhysRevD.93.082005

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.93.082005/fulltext

  • 22aAZ-3 計算機を利用したKAGRAの制御(VIII) Reviewed

    苔山 圭以子, 山本 尚弘, 譲原 浩貴, 宮川 治, 上泉 眞裕, 粟井 恭輔, 三代木 伸二, 道村 唯太, 端山 和大, 横澤 孝章, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集   71 ( 0 )   318 - 318   2016( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.71.1.0_537

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  • PROBING THE ROTATION OF CORE-COLLAPSE SUPERNOVA WITH A CONCURRENT ANALYSIS OF GRAVITATIONAL WAVES AND NEUTRINOS Reviewed

    Yokozawa Takaaki, Asano Mitsuhiro, Kayano Tsubasa, Suwa Yudai, Kanda Nobuyuki, Koshio Yusuke, Vagins Mark R.

    ASTROPHYSICAL JOURNAL   811 ( 2 )   2015.10( ISSN:0004-637X

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    DOI: 10.1088/0004-637X/811/2/86

  • PROBING THE ROTATION OF CORE-COLLAPSE SUPERNOVA WITH A CONCURRENT ANALYSIS OF GRAVITATIONAL WAVES AND NEUTRINOS Reviewed

    Takaaki Yokozawa, Mitsuhiro Asano, Tsubasa Kayano, Yudai Suwa, Nobuyuki Kanda, Yusuke Koshio, Mark R. Vagins

    ASTROPHYSICAL JOURNAL   811 ( 2 )   2015.10( ISSN:0004-637X ( eISSN:1538-4357

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    The next time a core-collapse supernova (SN) explodes in our galaxy, various detectors will be ready and waiting to detect its emissions of gravitational waves (GWs) and neutrinos. Current numerical simulations have successfully introduced multi-dimensional effects to produce exploding SN models, but thus far the explosion mechanism is not well understood. In this paper, we focus on an investigation of progenitor core rotation via comparison of the start time of GW emission and that of the neutronization burst. The GW and neutrino detectors are assumed to be, respectively, the KAGRA detector and a co-located gadolinium-loaded water Cherenkov detector, either EGADS or GADZOOKS!. Our detection simulation studies show that for a nearby SN (0.2 kpc) we can confirm the lack of core rotation close to 100% of the time, and the presence of core rotation about 90% of the time. Using this approach there is also the potential to confirm rotation for considerably more distant Milky Way SN explosions.

    DOI: 10.1088/0004-637X/811/2/86

  • Detectability of bigravity with graviton oscillations using gravitational wave observations Reviewed

    Narikawa Tatsuya, Ueno Koh, Tagoshi Hideyuki, Tanaka Takahiro, Kanda Nobuyuki, Nakamura Takashi

    PHYSICAL REVIEW D   91 ( 6 )   2015.03( ISSN:1550-7998

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    DOI: 10.1103/PhysRevD.91.062007

  • 22pDJ-13 Measurement of Schumann resonance in Kamioka Reviewed

    Atsuta Sho, Saito Yoshio, Somiya Kentaro, Nishizawa Atsushi, Miyakawa Osamu, Miyoki Shinji, Yano Kazushiro, Ogawa Tsutomu, Yamaguchi Satoru, HayamaC Kazuhiro, Araya Akito, Uyeshima Makoto, Uchiyama Takashi, Ono Kenji, Kanda Nobuyuki

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   70 ( 0 )   2015

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    DOI: 10.11316/jpsgaiyo.70.1.0_449

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  • 24pDJ-5 LSI Development and thermal design of Hard X-ray Monitor onboard WF-MAXI

    Vagins Mark

    The Physical Society of Japan (JPS), Meeting Abstracts of the Physical Society of Japan   70   504 - 504   2015( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.70.1.0_504

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  • 23pDM-13 Supernova ObservatioN NETwork based on the list of Supernova Progenitor IN our Galaxy

    Ohishi N., Tanaka M., Ishidoshiro K., Koshio Y., Tagoshi H., Kanda N.

    The Physical Society of Japan (JPS), Meeting Abstracts of the Physical Society of Japan   70   484 - 484   2015( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.70.1.0_484

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  • 23pDM-13 Supernova ObservatioN NETwork based on the list of Supernova Progenitor IN our Galaxy

    Ohishi N., Tanaka M., Ishidoshiro K., Koshio Y., Tagoshi H., Kanda N.

    Meeting Abstracts of the Physical Society of Japan   70   484 - 484   2015( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.70.1.0_484

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  • What can we learn from gravitational waves from nearby core-collapse supernovae?

    Yudai Suwa, Takaaki Yokozawa, Mitsuhiro Asano, Tsubasa Kayano, Nobuyuki Kanda, Yusuke Koshio, Mark R. Vagins

    SPANISH RELATIVITY MEETING (ERE 2014): ALMOST 100 YEARS AFTER EINSTEIN'S REVOLUTION   600   2015( ISSN:1742-6588 ( eISSN:1742-6596

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    Core-collapse supernova is one of the expected sources of gravitational wave (GW). The GW detection can be a smoking gun to probe the still unknown explosion mechanism. In the coming era of "multi-messenger astronomy", we can use photons, neutrinos and GW simultaneously to investigate these objects. By performing multi-dimensional simulations of neutrino-radiation hydrodynamics systematically, we calculate the gravitational wave and neutrino signals from nearby (galactic) core-collapse supernova. Based on these signals we will discuss the extractable information about the very central part of core-collapse supernovae.

    DOI: 10.1088/1742-6596/600/1/012009

  • 27pSK-5 Status of the development of data analysis pipeline for iKAGRA

    Tagoshi Hideyuki, Ueno Koh, Yuzurihara Hirotaka, Oohara Ken-ichi, Narikawa Tatsuya, Arima Tsukasa, Eda Kazunari, Fujii Yoshinori, Hayama Kazuhiro, Hiranuma Yuta, Hirobayashi Shigeki, Itoh Yousuke, Kanda Nobuyuki, Kaneyama Masato, Kim Jeongcho, Kim Chunglee, Lee Hyung Won, Mano Shuhei, Miyake Kyohei, Miyamoto Akinobu, Nakanishi Yuta, Nakano Masaya, Nakao Hayato, Ohishi Naoko, Sakai Kazuki, Sasaki Yukitsugu, Shoda Ayaka, Suwabe Hiroto, Takahashi Hirotaka, Tanaka Kazuyuki, Ueki Satoshi, Wakamatsu Takeshi, Yamamoto Takahiro, Yokoyama Jun'ichi, Yokozawa Takaaki

    Meeting Abstracts of the Physical Society of Japan   70   398 - 398   2015( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.70.2.0_398

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  • 27aSK-12 Control for KAGRA using digital system (VII)

    Miyakawa O., Kokeyama K., Kamiizumi M., Awai K., Miyoki S., Hayama K., Yokozawa T., Kanda N., Michimura Y., Yamamoto T., Yuzurihara H., KAGRA Collaboration

    Meeting Abstracts of the Physical Society of Japan   70   385 - 385   2015( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.70.2.0_385

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  • 24pDJ-5 LSI Development and thermal design of Hard X-ray Monitor onboard WF-MAXI

    Vagins Mark

    Meeting Abstracts of the Physical Society of Japan   70   504 - 504   2015( ISSN:2189-079X

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    DOI: 10.11316/jpsgaiyo.70.1.0_504

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  • Detectability of bigravity with graviton oscillations using gravitational wave observations Reviewed

    Tatsuya Narikawa, Koh Ueno, Hideyuki Tagoshi, Takahiro Tanaka, Nobuyuki Kanda, Takashi Nakamura

    Phys. Rev. D 91, 062007 (2015)   2014.12

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    The gravitational waveforms in the ghost-free bigravity theory exhibit<br />
    deviations from those in general relativity. The main difference is caused by<br />
    graviton oscillations in the bigravity theory. We investigate the prospects for<br />
    the detection of the corrections to gravitational waveforms from coalescing<br />
    compact binaries due to graviton oscillations and for constraining bigravity<br />
    parameters with the gravitational wave observations. We consider the bigravity<br />
    model discussed by the De Felice-Nakamura-Tanaka subset of the bigravity model,<br />
    and the phenomenological model in which the bigravity parameters are treated as<br />
    independent variables. In both models, the bigravity waveform shows strong<br />
    amplitude modulation, and there can be a characteristic frequency of the<br />
    largest peak of the amplitude, which depends on the bigravity parameters. We<br />
    show that there is a detectable region of the bigravity parameters for the<br />
    advanced ground-based laser interferometers, such as Advanced LIGO, Advanced<br />
    Virgo, and KAGRA. This region corresponds to the effective graviton mass of<br />
    $\mu \geq 10^{-17}~{\rm cm}^{-1}$ for $\tilde{c}-1 \geq 10^{-19}$ in the<br />
    phenomenological model, while $\mu \geq 10^{-16.5}~{\rm cm}^{-1}$ for<br />
    $\kappa\xi_c^2 \geq 10^{0.5}$ in the De Felice-Nakamura-Tanaka subset of the<br />
    bigravity model, respectively, where $\tilde{c}$ is the propagation speed of<br />
    the massive graviton and $\kappa\xi_c^2$ corresponds to the corrections to the<br />
    gravitational constant in general relativity. These regions are not excluded by<br />
    existing solar system tests. We also show that, in the case of $1.4-1.4M_{\rm<br />
    sun}$ binaries at the distance of $200~{\rm Mpc}$, $\log\mu^2$ is determined<br />
    with an accuracy of ${\cal O}$(0.1)\% at the 1$\sigma$ level for a fiducial<br />
    model with $\mu^2=10^{-33}~{\rm cm}^{-2}$ in the case of the phenomenological<br />
    model.

    DOI: 10.1103/PhysRevD.91.062007

  • Detectability and Parameter Estimation of Gravitational Waves from Cosmic String with Ground-Based Detectors

    Hirotaka Yuzurihara, Nobuyuki Kanda

    Proceedings of the 12th Asia Pacific Physics Conference (APPC12)   2014.03

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    Publishing type:Research paper (international conference proceedings)  

    DOI: 10.7566/jpscp.1.013117

  • Calibration and Reconstruction in Time-Series of Strain Signal of Gravitational Wave Detector

    Takahiro Yamamoto, Nobuyuki Kanda

    Proceedings of the 12th Asia Pacific Physics Conference (APPC12)   2014.03

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.7566/jpscp.1.013119

  • The cross-correlation search for a hot spot of gravitational waves : Numerical study for point spread function

    Yuta Okada, Nobuyuki Kanda, Sanjeev Dhurandhar, Hideyuki Tagoshi, Hirotaka Takahashi

    Journal of Physics: Conference Series   363   012040 - 012040   2012.06( eISSN:1742-6596

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    DOI: 10.1088/1742-6596/363/1/012040

  • LCGT and the global network of gravitational wave detectors

    Nobuyuki Kanda

    2011.12

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    Gravitational wave is a propagation of space-time distortion, which is predicted by Einstein in general relativity. Strong gravitational waves will come from some drastic astronomical objects, e.g. coalescence of neutron star binaries, black holes, supernovae, rotating pulsars and pulsar glitches. Detection of the gravitational waves from these objects will open a new door of \textit{`gravitational wave astronomy'}. Gravitational wave will be a probe to study the physics and astrophysics. To search these gravitational waves, large-scale laser interferometers will compose a global network of detectors. Advanced LIGO and advanced Virgo are upgrading from currents detectors. One of LIGO detector is considering to move Australia Site. IndIGO or Einstein Telescope are future plans. LCGT (Large-scale Cryogenic Gravitational wave Telescope) is now constructing in Japan with distinctive characters: cryogenic cooling mirror and underground site. We will present a design and a construction status of LCGT, and brief status of current gravitational wave detectors in the world. Network of these gravitational wave detectors will start in late 2016 or 2017, and may discover the gravitational waves. For example, these detectors will reach its search range for coalescence of neutron star binary is over 200 Mpc, and several or more events per year will be expected. Since most of gravitational wave events are from high-energy phenomenon of the astronomical objects, these might have counterpart evidences in electromagnetic radiation (visible light, X/gamma ray), neutrino, high energy particles or others. Thus, the mutual follow-up observations will give us more information of these objects.

  • Cross-correlation search for a hot spot of gravitational waves Reviewed

    Dhurandhar Sanjeev, Tagoshi Hideyuki, Okada Yuta, Kanda Nobuyuki, Takahashi Hirotaka

    PHYSICAL REVIEW D   84 ( 8 )   2011.10( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.84.083007

  • Cross-correlation search for a hot spot of gravitational waves Reviewed

    Dhurandhar Sanjeev, Tagoshi Hideyuki, Okada Yuta, Kanda Nobuyuki, Takahashi Hirotaka

    PHYSICAL REVIEW D   84 ( 8 )   2011.10( ISSN:2470-0010 ( eISSN:1550-2368

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    The cross-correlation search for gravitational wave, which is known as 'radiometry', has been previously applied to map of the gravitational wave stochastic background in the sky and also to target on gravitational wave from rotating neutron stars/pulsars. We consider the Virgo cluster where may be appear as `hot spot' spanning few pixels in the sky in radiometry analysis. Our results show that sufficient signal to noise ratio can be accumulated with integration times of the order of a year. We also construct numerical simulation of radiometry analysis, assuming current constructing/upgrading ground-based detectors. Point spread function of the injected sources are confirmed by numerical test. Typical resolution of radiometry analysis is a few square degree which corresponds to several thousand pixels of sky mapping.

    DOI: 10.1103/PhysRevD.84.083007

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.84.083007/fulltext

  • COHERENT VERSUS COINCIDENCE DETECTION OF GRAVITATIONAL WAVE SIGNALS FROM COMPACT INSPIRALING BINARIES Reviewed

    Dhurandhar S., Mukhopadhyay H., Tagoshi H., Kanda N.

    INTERNATIONAL JOURNAL OF MODERN PHYSICS D   20 ( 10 )   2051 - 2056   2011.09( ISSN:0218-2718

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1142/S0218271811020160

  • Coherent versus coincidence detection of gravitational wave signals from compact inspiraling binaries Reviewed

    S. Dhurandhar, H. Mukhopadhyay, H. Tagoshi, N. Kanda

    International Journal of Modern Physics D   20 ( 10 )   2051 - 2056   2011.09( ISSN:0218-2718

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    We compare two multi-detector detection strategies, namely, the coincidence and the coherent, for the detection of spinless inspiraling compact binary gravitational wave (GW) signals. The coincident strategy treats the detectors as if they are isolated, compares individual detector statistics with their respective thresholds, while the coherent strategy combines the detector network data phase coherently to obtain a single detection statistic which is then compared with a single threshold. In the case of geographically separated detectors, we also consider an enhanced coincidence strategy because the usual (naive) coincidence strategy yields poor results for misaligned detectors. For simplicity, we consider detector pairs having the same power spectral density of noise, as that of initial LIGO, and also assume the noise to be stationary and Gaussian. We compare the performances of the methods by plotting the receiver operating characteristic (ROC) for the two strategies. A single astrophysical source as well as a distribution of sources is considered. We find that the coherent strategy performs better than the two coincident strategies under the assumptions of stationary Gaussian detector noise. © 2011 World Scientific Publishing Company.

    DOI: 10.1142/S0218271811020160

  • The Japanese space gravitational wave antenna: DECIGO Reviewed

    Kawamura Seiji, Ando Masaki, Seto Naoki, Sato Shuichi, Nakamura Takashi, Tsubono Kimio, Kanda Nobuyuki, Tanaka Takahiro, Yokoyama Jun'ichi, Funaki Ikkoh, Numata Kenji, Ioka Kunihito, Takashima Takeshi, Agatsuma Kazuhiro, Akutsu Tomotada, Aoyanagi Koh-suke, Arai Koji, Araya Akito, Asada Hideki, Aso Yoichi, Chen Dan, Chiba Takeshi, Ebisuzaki Toshikazu, Ejiri Yumiko, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T., Ishidoshiro Koji, Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Izumi Kiwamu, Kawano Isao, Kawashima Nobuki, Kawazoe Fumiko, Kishimoto Naoko, Kiuchi Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Kuroyanagi Sachiko, Maeda Kei-ichi, Matsuhara Hideo, Matsumoto Nobuyuki, Michimura Yuta, Miyakawa Osamu, Miyamoto Umpei, Miyoki Shinji, Morimoto Mutsuko Y., Morisawa Toshiyuki, Moriwaki Shigenori, Mukohyama Shinji, Musha Mitsuru, Nagano Shigeo, Naito Isao, Nakamura Kouji, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nakazawa Kazuhiro, Nishida Erina, Nishiyama Kazutaka, Nishizawa Atsushi, Niwa Yoshito, Noumi Taiga, Obuchi Yoshiyuki, Ohashi Masatake, Ohishi Naoko, Ohkawa Masashi, Okada Kenshi, Okada Norio, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Saito Ryo, Sakagami Masaaki, Sakai Shin-ichiro, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shinkai Hisaaki, Shoda Ayaka, Somiya Kentaro, Sotani Hajime, Sugiyama Naoshi, Suwa Yudai, Suzuki Rieko, Tagoshi Hideyuki, Takahashi Fuminobu, Takahashi Kakeru, Takahashi Keitaro, Takahashi Ryutaro, Takahashi Ryuichi, Takahashi Tadayuki, Takahashi Hirotaka, Akiteru Takamori, Takano Tadashi, Tanaka Nobuyuki, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Torii Yasuo, Toyoshima Morio, Tsujikawa Shinji, Tsunesada Yoshiki, Ueda Akitoshi, Ueda Ken-ichi, Utashima Masayoshi, Wakabayashi Yaka, Yagi Kent, Yamakawa Hiroshi, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh, Sun Ke-Xun

    CLASSICAL AND QUANTUM GRAVITY   28 ( 9 )   2011.05( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/28/9/094011

  • The Japanese space gravitational wave antenna: DECIGO

    Seiji Kawamura, Seiji Kawamura, Masaki Ando, Naoki Seto, Shuichi Sato, Takashi Nakamura, Kimio Tsubono, Nobuyuki Kanda, Takahiro Tanaka, Jun'Ichi Yokoyama, Ikkoh Funaki, Kenji Numata, Kunihito Ioka, Takeshi Takashima, Kazuhiro Agatsuma, Tomotada Akutsu, Koh Suke Aoyanagi, Koji Arai, Akito Araya, Hideki Asada, Yoichi Aso, Dan Chen, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki T. Inoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Kiwamu Izumi, Isao Kawano, Nobuki Kawashima, Fumiko Kawazoe, Naoko Kishimoto, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Sachiko Kuroyanagi, Kei Ichi Maeda, Hideo Matsuhara, Nobuyuki Matsumoto, Yuta Michimura, Osamu Miyakawa, Umpei Miyamoto, Shinji Miyoki, Mutsuko Y. Morimoto, Toshiyuki Morisawa, Shigenori Moriwaki, Shinji Mukohyama, Mitsuru Musha, Shigeo Nagano, Isao Naito, Kouji Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Kazuhiro Nakazawa, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Naoko Ohishi, Masashi Ohkawa, Kenshi Okada, Norio Okada

    Classical and Quantum Gravity   28 ( 9 )   2011.05( ISSN:0264-9381 ( eISSN:1361-6382

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    The objectives of the DECi-hertz Interferometer Gravitational Wave Observatory (DECIGO) are to open a new window of observation for gravitational wave astronomy and to obtain insight into significant areas of science, such as verifying and characterizing inflation, determining the thermal history of the universe, characterizing dark energy, describing the formation mechanism of supermassive black holes in the center of galaxies, testing alternative theories of gravity, seeking black hole dark matter, understanding the physics of neutron stars and searching for planets around double neutron stars. DECIGO consists of four clusters of spacecraft in heliocentric orbits; each cluster employs three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by three pairs of differential Fabry-Perot Michelson interferometers. Two milestone missions, DECIGO pathfinder and Pre-DECIGO, will be launched to demonstrate required technologies and possibly to detect gravitational waves. © 2011 IOP Publishing Ltd.

    DOI: 10.1088/0264-9381/28/9/094011

  • Upper Limit on Gravitational Wave Backgrounds at 0.2 Hz with a Torsion-Bar Antenna Reviewed

    Ishidoshiro Koji, Ando Masaki, Takamori Akiteru, Takahashi Hirotaka, Okada Kenshi, Matsumoto Nobuyuki, Kokuyama Wataru, Kanda Nobuyuki, Aso Yoichi, Tsubono Kimio

    PHYSICAL REVIEW LETTERS   106 ( 16 )   2011.04( ISSN:0031-9007

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevLett.106.161101

  • Upper Limit on Gravitational Wave Backgrounds at 0.2 Hz with a Torsion-Bar Antenna Reviewed

    Koji Ishidoshiro, Masaki Ando, Akiteru Takamori, Hirotaka Takahashi, Kenshi Okada, Nobuyuki Matsumoto, Wataru Kokuyama, Nobuyuki Kanda, Yoichi Aso, Kimio Tsubono

    Physical Review Letter   106 ( 16 )   161101   2011.04( ISSN:0031-9007 ( eISSN:1079-7114

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  • Prospects for true calorimetry on Kerr black holes in core-collapse supernovae and mergers Reviewed

    van Putten Maurice H. P. M., Kanda Nobuyuki, Tagoshi Hideyuki, Tatsumi Daisuke, Masa-Katsu Fujimoto, Della Valle Massimo

    PHYSICAL REVIEW D   83 ( 4 )   2011.02( ISSN:1550-7998

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.83.044046

  • Prospects for true calorimetry on Kerr black holes in core-collapse supernovae and mergers Reviewed

    Maurice H. P. M. Van Putten, Nobuyuki Kanda, Hideyuki Tagoshi, Daisuke Tatsumi, Fujimoto Masa-Katsu, Massimo Della Valle

    Physical Review D - Particles, Fields, Gravitation and Cosmology   83 ( 4 )   2011.02( ISSN:1550-7998

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    Observational evidence for black hole spin down has been found in the normalized light curves of long gamma-ray bursts in the BATSE catalog. Over the duration T90 of the burst, matter swept up by the central black hole is susceptible to nonaxisymmetries, producing gravitational radiation with a negative chirp. A time-sliced matched filtering method is introduced to capture phase coherence on intermediate time scales, τ, here tested by the injection of templates into experimental strain noise, hn(t). For TAMA 300, hn(f) 10-21Hz-1/2 at f=1kHz gives a sensitivity distance for a reasonably accurate extraction of the trajectory in the time-frequency domain of about D 0.07-0.10Mpc for the spin down of black holes of mass M=10-12M with τ=1s. Extrapolation to advanced detectors implies D 35-50Mpc for hn(f) 2×10-24Hz -1/2 around 1 kHz, which will open a new window to rigorous calorimetry on Kerr black holes. © 2011 American Physical Society.

    DOI: 10.1103/PhysRevD.83.044046

  • DECIGO and DECIGO pathfinder Reviewed

    Ando Masaki, Kawamura Seiji, Seto Naoki, Sato Shuichi, Nakamura Takashi, Tsubono Kimio, Takashima Takeshi, Funaki Ikkoh, Numata Kenji, Kanda Nobuyuki, Tanaka Takahiro, Ioka Kunihito, Agatsuma Kazuhiro, Aoyanagi Koh-suke, Arai Koji, Araya Akito, Asada Hideki, Aso Yoichi, Chiba Takeshi, Ebisuzaki Toshikazu, Ejiri Yumiko, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T., Ishidoshiro Koji, Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Izumi Kiwamu, Kawano Isao, Kawashima Nobuki, Kawazoe Fumiko, Kishimoto Naoko, Kiuchi Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Maeda Kei-ichi, Matsuhara Hideo, Mino Yasushi, Miyakawa Osamu, Miyamoto Umpei, Miyoki Shinji, Morimoto Mutsuko Y., Morisawa Toshiyuki, Moriwaki Shigenori, Mukohyama Shinji, Musha Mitsuru, Nagano Shigeo, Naito Isao, Nakamura Kouji, Nakamura Masahiro, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nakazawa Kazuhiro, Nishida Erina, Nishiyama Kazutaka, Nishizawa Atsushi, Niwa Yoshito, Noumi Taiga, Obuchi Yoshiyuki, Ohashi Masatake, Ohishi Naoko, Ohkawa Masashi, Okada Kenshi, Okada Norio, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Saito Ryo, Sakagami Masaaki, Sakai Shin-ichiro, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shinkai Hisaaki, Somiya Kentaro, Sotani Hajime, Sugiyama Naoshi, Suwa Yudai, Suzuki Rieko, Tagoshi Hideyuki, Takahashi Fuminobu, Takahashi Kakeru, Takahashi Keitaro, Takahashi Ryutaro, Takahashi Ryuichi, Takahashi Tadayuki, Takahashi Hirotaka, Akiteru Takamori, Takano Tadashi, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Torii Yasuo, Toyoshima Morio, Tsujikawa Shinji, Tsunesada Yoshiki, Ueda Akitoshi, Ueda Ken-ichi, Utashima Masayoshi, Wakabayashi Yaka, Yagi Kent, Yamakawa Hiroshi, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yokoyama Jun'ichi, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh, Sun Ken-Xun

    CLASSICAL AND QUANTUM GRAVITY   27 ( 8 )   2010.04( ISSN:0264-9381

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1088/0264-9381/27/8/084010

  • DECIGO and DECIGO pathfinder

    Masaki Ando, Seiji Kawamura, Naoki Seto, Shuichi Sato, Takashi Nakamura, Kimio Tsubono, Takeshi Takashima, Ikkoh Funaki, Kenji Numata, Nobuyuki Kanda, Takahiro Tanaka, Kunihito Ioka, Kazuhiro Agatsuma, Koh Suke Aoyanagi, Koji Arai, Akito Araya, Hideki Asada, Yoichi Aso, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki T. Inoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Kiwamu Izumi, Isao Kawano, Nobuki Kawashima, Fumiko Kawazoe, Naoko Kishimoto, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Kei Ichi Maeda, Hideo Matsuhara, Yasushi Mino, Osamu Miyakawa, Umpei Miyamoto, Shinji Miyoki, Mutsuko Y. Morimoto, Toshiyuki Morisawa, Shigenori Moriwaki, Shinji Mukohyama, Mitsuru Musha, Shigeo Nagano, Isao Naito, Kouji Nakamura, Masahiro Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Kazuhiro Nakazawa, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Masashi Ohkawa, Kenshi Okada, Norio Okada, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Ryo Saito, Masaaki Sakagami, Shin Ichiro Sakai

    Classical and Quantum Gravity   27 ( 8 )   2010.04( ISSN:0264-9381 ( eISSN:1361-6382

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    A space gravitational-wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory), will provide fruitful insights into the universe, particularly on the formation mechanism of supermassive black holes, dark energy and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprising four interferometer units; each interferometer unit will be formed by three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight with long baseline, it is important to increase the technical feasibility before its planned launch in 2027. Thus, we are planning to launch two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission, and key components for DPF are being tested on ground and in orbit. In this paper, we review the conceptual design and current status of DECIGO and DPF. © 2010 IOP Publishing Ltd.

    DOI: 10.1088/0264-9381/27/8/084010

  • 21pBL-7 Current Status and Future of Gravitational Wave Detectors Reviewed

    Kanda Nobuyuki

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   65 ( 0 )   2010

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    Publishing type:Research paper (scientific journal)   Kind of work:Single Work  

    DOI: 10.11316/jpsgaiyo.65.1.1.0_116_2

    CiNii Article

  • DECIGO: the Japanese Space Gravitational Wave Antenna Reviewed

    ANDO Masaki, MORIWAKI Shigenori, MUSHA Mitsuru, NAKAZAWA Kazuhiro, NUMATA Kenji, SAKAI Shin-ichiro, SETO Naoki, TAKASHIMA Takeshi, TANAKA Takahiro, DECIGO Working Group the, KAWAMURA Seiji, SATO Shuichi, NAKAMURA Takashi, TSUBONO Kimio, ARAYA Akito, FUNAKI Ikkoh, IOKA Kunihito, KANDA Nobuyuki

    一般社団法人 日本航空宇宙学会 TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, AEROSPACE TECHNOLOGY JAPAN   8 ( 27 )   Po_4_1 - Po_4_6   2010

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    A space gravitational wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory) will provide fruitful insights into the universe, particularly on dark energy, the formation mechanism of supermassive black holes, and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprised of 4 interferometer units; each interferometer unit will be realized by formation flight of three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight, it is important to increase the technical feasibility before its planned launch in 2024. Thus, we are planning two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission for DECIGO, and key components for DPF are being tested on ground and in orbit. In this article, we review the conceptual design and current status of DECIGO and DPF.

    DOI: 10.2322/tastj.8.Po_4_1

    CiNii Article

  • DECIGO: the Japanese Space Gravitational Wave Antenna

    ANDO Masaki, KAWAMURA Seiji, SATO Shuichi, NAKAMURA Takashi, TSUBONO Kimio, ARAYA Akito, FUNAKI Ikkoh, IOKA Kunihito, KANDA Nobuyuki, MORIWAKI Shigenori, MUSHA Mitsuru, NAKAZAWA Kazuhiro, NUMATA Kenji, SAKAI Shin-ichiro, SETO Naoki, TAKASHIMA Takeshi, TANAKA Takahiro, DECIGO Working Group the

    TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, SPACE TECHNOLOGY JAPAN   8 ( 27 )   Po_4_1 - Po_4_6   2010( ISSN:1884-0485 ( eISSN:18840485

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    A space gravitational wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory) will provide fruitful insights into the universe, particularly on dark energy, the formation mechanism of supermassive black holes, and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprised of 4 interferometer units; each interferometer unit will be realized by formation flight of three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight, it is important to increase the technical feasibility before its planned launch in 2024. Thus, we are planning two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission for DECIGO, and key components for DPF are being tested on ground and in orbit. In this article, we review the conceptual design and current status of DECIGO and DPF.

    DOI: 10.2322/tastj.8.Po_4_1

    CiNii Article

  • Detecting gravitational waves from inspiraling binaries with a network of geographically separated detectors: Coherent versus coincident strategies Reviewed

    Mukhopadhyay Himan, Tagoshi Hideyuki, Dhurandhar Sanjeev, Kanda Nobuyuki

    PHYSICAL REVIEW D   80 ( 12 )   2009.12( ISSN:1550-7998

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    DOI: 10.1103/PhysRevD.80.123019

  • Detecting gravitational waves from inspiraling binaries with a network of geographically separated detectors: Coherent versus coincident strategies Reviewed

    Himan Mukhopadhyay, Hideyuki Tagoshi, Sanjeev Dhurandhar, Nobuyuki Kanda

    PHYSICAL REVIEW D   80 ( 12 )   2009.12( ISSN:1550-7998

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    We compare two strategies of multidetector detection of compact binary inspiral signals, namely, the coincidence and the coherent for the realistic case of geographically separated detectors. The naive coincident strategy treats the detectors as if they are isolated-compares individual detector statistics with their respective thresholds while the coherent strategy combines the detector network data coherently to obtain a single detection statistic which is then compared with a single threshold. We also consider an enhanced coincidence strategy which is intermediate in the sense that though the individual statistics are added in quadrature and the sum compared with a single threshold, the estimated parameters are also checked for consistency. For simplicity, we consider detector pairs having the same power spectral density of noise, as that of initial LIGO and also assume the noise to be stationary and Gaussian. Further, since we consider the detectors to be widely separated on Earth, we take the instrumental noises to be uncorrelated; the wide separation implicitly means that since the detector arms must lie parallel to the Earth&apos;s surface, the detectors necessarily have different orientations. We compare the performances of the methods by plotting the receiver operating characteristics for the strategies. Several results are derived analytically in order to gain insight. Simulations are performed in order to plot the receiver operating characteristic (ROC) curves. A single astrophysical source as well as a distribution of sources is considered. We assume a 1 yr data train and a mass range of 1-40M(circle dot) for the case of astrophysically distributed sources. We find that the coherent strategy is superior to the two coincident strategies that we consider. Remarkably, the detection probability of the coherent strategy is 50% better than the naive coincident strategy. One the other hand, the difference in performance between the coherent strategy and enhanced coincident strategy is not very large. Even in this situation, it is not difficult to perform the real data analysis with the coherent strategy. The bottom line is that the coherent strategy is a good detection strategy.

    DOI: 10.1103/PhysRevD.80.123019

  • DECIGO: The Japanese space gravitational wave antenna

    Shuichi Sato, Seiji Kawamura, Masaki Ando, Takashi Nakamura, Kimio Tsubono, Akito Araya, Ikkoh Funaki, Kunihito Ioka, Nobuyuki Kanda, Shigenori Moriwaki, Mitsuru Musha, Kazuhiro Nakazawa, Kenji Numata, Shin Ichiro Sakai, Naoki Seto, Takeshi Takashima, Takahiro Tanaka, Kazuhiro Agatsuma, Koh Suke Aoyanagi, Koji Arai, Hideki Asada, Yoichi Aso, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Katsuhiko Ganzu, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki TInoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Nobuki Kawashima, Fumiko Kawazoe, Kishimoto Naoko, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hideaki Kudoh, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Kei Ichi Maeda, Hideo Matsuhara, Yasushi Mino, Osamu Miyakawa, Shinji Miyoki, Mutsuko YMorimoto, Tomoko Morioka, Toshiyuki Morisawa, Shinji Mukohyama, Shigeo Nagano, Isao Naito, Kouji Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Masashi Ohkawa, Norio Okada, Kouji Onozato, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Masaaki Sakagami, Shihori Sakata, Misao Sasaki

    Journal of Physics: Conference Series   154   2009.06( ISSN:1742-6588 ( eISSN:1742-6596

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    DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a differential Fabry-Perot interferometer. We plan to launch DECIGO in middle of 2020s, after sequence of two precursor satellite missions, DECIGO pathfinder and Pre-DECIGO, for technology demonstration required to realize DECIGO and hopefully for detection of gravitational waves from our galaxy or nearby galaxies. © 2009 IOP Publishing Ltd.

    DOI: 10.1088/1742-6596/154/1/012040

  • DECIGO pathfinder Reviewed

    Ando Masaki, Kawamura Seiji, Sato Shuichi, Nakamura Takashi, Tsubono Kimio, Araya Akito, Funaki Ikkoh, Ioka Kunihito, Kanda Nobuyuki, Moriwaki Shigenori, Musha Mitsuru, Nakazawa Kazuhiro, Numata Kenji, Sakai Shin-ichiro, Seto Naoki, Takashima Takeshi, Tanaka Takahiro, Agatsuma Kazuhiro, Aoyanagi Koh-suke, Arai Koji, Asada Hideki, Aso Yoichi, Chiba Takeshi, Ebisuzaki Toshikazu, Ejiri Yumiko, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Ganzu Katsuhiko, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T., Ishidoshiro Koji, Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Kawashima Nobuki, Kawazoe Fumiko, Kishimoto Naoko, Kiuchi Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kudoh Hideaki, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Maeda Kei-ichi, Matsuhara Hideo, Mino Yasushi, Miyakawa Osamu, Miyoki Shinji, Morimoto Mutsuko Y., Morioka Tomoko, Morisawa Toshiyuki, Mukohyama Shinji, Nagano Shigeo, Naito Isao, Nakamura Kouji, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nishida Erina, Nishiyama Kazutaka, Nishizawa Atsushi, Niwa Yoshito, Noumi Taiga, Obuchi Yoshiyuki, Ohashi Masatake, Ohishi Naoko, Ohkawa Masashi, Okada Norio, Onozato Kouji, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Sakagami Masaaki, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shinkai Hisaaki, Somiya Kentaro, Sotani Hajime, Sugiyama Naoshi, Suwa Yudai, Suzuki Rieko, Tagoshi Hideyuki, Takahashi Fuminobu, Takahashi Kakeru, Takahashi Keitaro, Takahashi Ryutaro, Takahashi Ryuichi, Takahashi Tadayuki, Takahashi Hirotaka, Akiteru Takamori, Takano Tadashi, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Torii Yasuo, Toyoshima Morio, Tsujikawa Shinji, Tsunesada Yoshiki, Ueda Akitoshi, Ueda Ken-ichi, Utashima Masayoshi, Wakabayashi Yaka, Yamakawa Hiroshi, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yokoyama Jun'ichi, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh

    CLASSICAL AND QUANTUM GRAVITY   26 ( 9 )   2009.05( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/26/9/094019

  • DECIGO pathfinder Reviewed

    Masaki Ando, Seiji Kawamura, Shuichi Sato, Takashi Nakamura, Kimio Tsubono, Akito Araya, Ikkoh Funaki, Kunihito Ioka, Nobuyuki Kanda, Shigenori Moriwaki, Mitsuru Musha, Kazuhiro Nakazawa, Kenji Numata, Shin-ichiro Sakai, Naoki Seto, Takeshi Takashima, Takahiro Tanaka, Kazuhiro Agatsuma, Koh-suke Aoyanagi, Koji Arai, Hideki Asada, Yoichi Aso, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa-Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Katsuhiko Ganzu, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng-Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki T. Inoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Nobuki Kawashima, Fumiko Kawazoe, Naoko Kishimoto, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hideaki Kudoh, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Kei-ichi Maeda, Hideo Matsuhara, Yasushi Mino, Osamu Miyakawa, Shinji Miyoki, Mutsuko Y. Morimoto, Tomoko Morioka, Toshiyuki Morisawa, Shinji Mukohyama, Shigeo Nagano, Isao Naito, Kouji Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Masashi Ohkawa, Norio Okada, Kouji Onozato, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Masaaki Sakagami, Shihori Sakata, Misao Sasaki, Takashi Sato, Masaru Shibata, Hisaaki Shinkai, Kentaro Somiya, Hajime Sotani, Naoshi Sugiyama, Yudai Suwa, Rieko Suzuki, Hideyuki Tagoshi, Fuminobu Takahashi, Kakeru Takahashi, Keitaro Takahashi, Ryutaro Takahashi, Ryuichi Takahashi, Tadayuki Takahashi, Hirotaka Takahashi, Takamori Akiteru, Tadashi Takano, Keisuke Taniguchi, Atsushi Taruya, Hiroyuki Tashiro, Yasuo Torii, Morio Toyoshima, Shinji Tsujikawa, Yoshiki Tsunesada, Akitoshi Ueda, Ken-ichi Ueda, Masayoshi Utashima, Yaka Wakabayashi, Hiroshi Yamakawa, Kazuhiro Yamamoto, Toshitaka Yamazaki, Jun'ichi Yokoyama, Chul-Moon Yoo, Shijun Yoshida, Taizoh Yoshino

    CLASSICAL AND QUANTUM GRAVITY   26 ( 9 )   2009.05( ISSN:0264-9381 ( eISSN:1361-6382

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    DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory), which is a future space gravitational wave antenna. DECIGO is expected to provide fruitful insights into the universe, particularly about dark energy, the formation mechanism of supermassive black holes and the inflation of the universe. Since DECIGO will be an extremely challenging mission, which will be formed by three drag-free spacecraft with 1000 km separation, it is important to increase the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. In this paper, we review the conceptual design and current status of the first milestone mission, DPF.

    DOI: 10.1088/0264-9381/26/9/094019

  • Astrophysically motivated time-frequency clustering for burst gravitational wave search: application to TAMA300 data Reviewed

    Honda Ryota, Yamagishi Shougo, Kanda Nobuyuki

    CLASSICAL AND QUANTUM GRAVITY   25 ( 18 )   2008.09( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/25/18/184035

  • Search for continuous gravitational waves from PSR J0835-4510 using CLIO data Reviewed

    Akutsu Tomomi, Ando Masaki, Haruyama Tomiyoshi, Kanda Nobuyuki, Kuroda Kazuaki, Miyoki Sinji, Ohashi Masatake, Saito Yoshio, Sato Nobuaki, Shintomi Takakazu, Suzuki Toshikazu, Tagoshi Hideyuki, Takahashi Hirotaka, Tatsumi Daisuke, Telada Souichi, Tomaru Takayuki, Uchiyama Takashi, Yamamoto Akira, Yamamoto Kazuhiro

    CLASSICAL AND QUANTUM GRAVITY   25 ( 18 )   2008.09( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/25/18/184013

  • Astrophysically motivated time-frequency clustering for burst gravitational wave search: application to TAMA300 data Reviewed

    Ryota Honda, Shougo Yamagishi, Nobuyuki Kanda

    CLASSICAL AND QUANTUM GRAVITY   25 ( 18 )   2008.09( ISSN:0264-9381 ( eISSN:1361-6382

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    We have developed a method of 'time-frequency (TF) clustering' to find burst gravitational waves for TAMA data analysis. The TF clustering method on the sonogram (spectrogram) shows some characteristics of short-duration signals. Burst gravitational waveforms from stellar-core collapse of supernovae that are predicted by Dimmelmeier et al [1, 2] (DFM waveforms) have short durations on the order of 10 ms and have a large spike and ringing tail in time series. On the other hand, typical detector instrumental noise transients of the same timescale have different waveforms as like as simpler spikes. Since the numerically predicted waveforms may not be reliable given conditions and model dependency, using one search algorithm is not robust to differentiate gravitational waves from instrumental noises. Our proposal for performing the separation is to compare many parameters of the cluster that represent the signal waveform. This approach will be useful for cases when the difference between gravitational waves and noise is not clear for one parameter. We employ TF clustering to represent the waveform characteristics. We calculated the parameters of each respective cluster, such as the magnitude and the Nth momentum around the center of a power distribution of the cluster. Using these parameters, we can efficiently identify some predicted gravitational waveforms and can exclude the TAMA detector's typical unstable spike-like noises due to the instruments. Our selection criteria for TF cluster shape parameters achieved an average efficiency of roughly 50% for injected DFM waveforms of h(rss) similar to 2 x 10(-20) Hz(-1/2) (source distance of 350 pc) with false alarm rate of similar to 1 Hz. In addition, the false alarm rate for larger noises, such as SNR &gt; 100, is improved 10-fold by applying the selection criteria for TF cluster parameters.

    DOI: 10.1088/0264-9381/25/18/184035

  • Effect of energy deposited by cosmic-ray particles on interferometric gravitational wave detectors Reviewed

    Yamamoto Kazuhiro, Hayakawa Hideaki, Okada Atsushi, Uchiyama Takashi, Miyoki Shinji, Ohashi Masatake, Kuroda Kazuaki, Kanda Nobuyuki, Tatsumi Daisuke, Tsunesada Yoshiki

    PHYSICAL REVIEW D   78 ( 2 )   2008.07( ISSN:1550-7998

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    DOI: 10.1103/PhysRevD.78.022004

  • Effect of energy deposited by cosmic-ray particles on interferometric gravitational wave detectors Reviewed

    Kazuhiro Yamamoto, Hideaki Hayakawa, Atsushi Okada, Takashi Uchiyama, Shinji Miyoki, Masatake Ohashi, Kazuaki Kuroda, Nobuyuki Kanda, Daisuke Tatsumi, Yoshiki Tsunesada

    Phys.Rev.D78:022004,2008   78 ( 2 )   2008.05( ISSN:1550-7998 ( eISSN:1550-2368

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    Publishing type:Research paper (scientific journal)   International / domestic magazine:International journal  

    We investigated the noise of interferometric gravitational wave detectors due<br />
    to heat energy deposited by cosmic-ray particles. We derived a general formula<br />
    that describes the response of a mirror against a cosmic-ray passage. We found<br />
    that there are differences in the comic-ray responses (the dependence of<br />
    temperature and cosmic-ray track position) in cases of interferometric and<br />
    resonant gravitational wave detectors. The power spectral density of vibrations<br />
    caused by low-energy secondary muons is 100-times smaller than the goal<br />
    sensitivity of future second-generation interferometer projects, such as LCGT<br />
    and Advanced LIGO. The arrival frequency of high-energy cosmic-ray muons that<br />
    generate enough large showers inside mirrors of LCGT and Advanced LIGO is one<br />
    per a millennium. We also discuss the probability of exotic-particle detection<br />
    with interferometers.

    DOI: 10.1103/PhysRevD.78.022004

  • Time-frequency clustering for burst gravitational waves search in TAMA300 data

    Nobuyuki Kanda

    2008.04

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    We have developed a method 'time-frequency (TF) clustering' to find the burst gravitational waves for TAMA data analysis. TF clustering method on sonogram (spectrogram) shows some characteristics of short duration signal. Using parameters which represent the cluster shape, we can efficiently identify some predicted gravitational wave forms and can exclude typical unstable spike like noises due to detector instruments. The requirement of some parameters of cluster achieved roughly 50% average efficiency for injected DFM waveforms of $h_{rss}\sim 2 \times 10^{-19}$ for type I burst. Also the reduction for signal by spike noises are more than one order improvement for the SNR$ > $100.

  • 24pZW-2 Status of Development for Interferometric Gravitational Wave Detector TAMA300 XX (Interferometer Development) Reviewed

    Arai K., Ishizaki H., Nakagawa N., Takamori A., Bertolini A., DeSalvo R., Sato S., Aso Y., Akutsu T., Tsunesada Y., Nagano S., Tatsumi D., Ando M., Miyoki S., Moriwaki S., Kanda N., Musha M., Fujimoto M.-K., Kawamura S., Mio N., Ohashi M., Kuroda K., Takahashi R., Tsubono K., TAMA Conaboration, Izumi K., Agatsuma K., Arase Y., Wakabayashi Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   63 ( 0 )   2008

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    DOI: 10.11316/jpsgaiyo.63.1.1.0_112_1

    CiNii Article

  • Search for gravitational waves on short duration in TAMA300 data : stellar core collapse and black hole Reviewed

    Ryota Honda, Nobuyuki Kanda, Tomomi Akutsu, Masaki Ando, Yoshiki Tsunesada

    IOP PUBLISHING LTD TAUP2007: TENTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS   120   2008( ISSN:1742-6588

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    We present in the results of TAMA300 data analysis for short duration gravitational waves. The excess power filter, alternative linear filter (ALF) and TF(time-frequency) clustering methods have been employed for burst gravitational waves from stellar-core collapse, and matched filtering method used for the ringdown gravitational waves from black hole quasi-normal oscillations. The observational range of TAMA for the burst gravitational waves is roughly 1 kpc, and the range for black hole ringdown covers most of our galaxy. We have been developed new method 'time-frequency (TF) clustering' to find the burst waves. This is a TF clustering method on spectrogram (sonogram). Using this method, we can efficiently identify some predicted gravitational wave forms[2] and can exclude typical unstable spike like noises.

    DOI: 10.1088/1742-6596/120/3/032013

  • DECIGO Pathfinder Reviewed

    Ando Masaki, Kawamura Seiji, Nakamura Takashi, Tsubono Kimio, Tanaka Takahiro, Funaki Ikkoh, Seto Naoki, Numata Kenji, Sato Shuichia, Ioka Kunihito, Kanda Nobuyuki, Takashima Takeshi, Agatsuma Kazuhiro, Akutsu Tomotada, Akutsu Tomomi, Aoyanagi Koh-suke, Arai Koji, Arase Yuta, Araya Akito, Asada Hideki, Aso Yoichi, Chiba Takeshi, Ebisuzaki Toshikazu, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Ganzu Katsuhiko, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T, Ishidoshiro Koji, Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Kamagasako Shogo, Kawashima Nobuki, Kawazoe Fumiko, Kirihara Hiroyuki, Kishimoto Naoko, Kiuche Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kudoh Hideaki, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Maeda Kei-ichi, Matsuhara Hideo, Mino Yasushi, Miyakawa Osamu, Miyoki Shinji, Morimoto Mutsuko Y, Morioka Tomoko, Morisawa Toshiyuki, Moriwaki Shigenori, Mukohyama Shinji, Musha Mitsuru, Nagano Shigeo, Naito Isao, Nakagawa Noriyasu, Nakamura Kouji, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nishida Erina, Nishiyama Kazutaka, Nishizawa Atsushi, Niwa Yoshito, Ohashi Masatake, Ohishi Naoko, Ohkawa Masashi, Okutomi Akira, Onozato Kouji, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Sakagami Masaaki, Sakai Shin-ichiro, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shinkai Hisaaki, Somiya Kentaro, Sotani Hajime, Sugiyama Naoshi, Suwa Yudai, Tagoshi Hideyuki, Takahashi Kakeru, Takahashi Keitaro, Takahashi Tadayuki, Takahashi Hirotaka, Takahashi Ryuichi, Takahashi Ryutaro, Takamori Akiteru, Takano Tadashi, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Tokuda Mitsuru, Tokunari Masao, Toyoshima Morio, Tsujikawa Shinji, Tsunesada Yoshiki, Ueda Ken-ichi, Utashima Masayoshi, Yamakawa Hiroshi, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yokoyama Jun'ichi, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh

    TAUP2007: TENTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS   120   2008( ISSN:1742-6588

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    DOI: 10.1088/1742-6596/120/3/032005

  • The Japanese space gravitational wave antenna - DECIGO Reviewed

    S. Kawamura, M. Ando, T. Nakamura, K. Tsubono, T. Tanaka, I. Funaki, N. Seto, K. Numata, S. Sato, K. Ioka, N. Kanda, T. Takashima, K. Agatsuma, T. Akutsu, T. Akutsu, K.-S. Aoyanagi, K. Arai, Y. Arase, A. Araya, H. Asada, Y. Aso, T. Chiba, T. Ebisuzaki, M. Enoki, Y. Eriguchi, M.-K. Fujimoto, R. Fujita, M. Fukushima, T. Futamase, K. Ganzu, T. Harada, T. Hashimoto, K. Hayama, W. Hikida, Y. Himemoto, H. Hirabayashi, T. Hiramatsu, F.-L. Hong, H. Horisawa, M. Hosokawa, K. Ichiki, T. Ikegami, K.T. Inoue, K. Ishidoshiro, H. Ishihara, T. Ishikawa, H. Ishizaki, H. Ito, Y. Itoh, S. Kamagasako, N. Kawashima, F. Kawazoe, H. Kirihara, N. Kishimoto, K. Kiuchi, S. Kobayashi, K. Kohri, H. Koizumi, Y. Kojima, K. Kokeyama, W. Kokuyama, K. Kotake, Y. Kozai, H. Kudoh, H. Kunimori, H. Kuninaka, K. Kuroda, K.-I. Maeda, H. Matsuhara, Y. Mino, O. Miyakawa, S. Miyoki, Y. Morimoto, T. Morioka, T. Morisawa, S. Moriwaki, S. Mukohyama, M. Musha, S. Nagano, I. Naito, N. Nakagawa, K. Nakamura, H. Nakano, K. Nakao, S. Nakasuka, Y. Nakayama, E. Nishida, K. Nishiyama, A. Nishizawa, Y. Niwa, M. Ohashi, N. Ohishi, M. Ohkawa, A. Okutomi, K. Onozato, K. Oohara, N. Sago, M. Saijo, M. Sakagami, S.-I. Sakai, S. Sakata, M. Sasaki, T. Sato, M. Shibata, H. Shinkai, K. Somiya, H. Sotani, N. Sugiyama, Y. Suwa, H. Tagoshi, K. Takahashi, K. Takahashi, T. Takahashi, H. Takahashi, R. Takahashi, R. Takahashi, A. Takamori, T. Takano, K. Taniguchi, A. Taruya, H. Tashiro, M. Tokuda, M. Tokunari, M. Toyoshima, S. Tsujikawa, Y. Tsunesada, K.-I. Ueda, M. Utashima, H. Yamakawa, K. Yamamoto, T. Yamazaki, J. Yokoyama, C.-M. Yoo, S. Yoshida, T. Yoshino

    Journal of Physics: Conference Series   122   012006 - 012006   2008( eISSN:1742-6596

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    DOI: 10.1088/1742-6596/122/1/012006

  • Search for gravitational waves on short duration in TAMA300 data : stellar core collapse and black hole Reviewed

    Ryota Honda, Nobuyuki Kanda, Tomomi Akutsu, Masaki Ando, Yoshiki Tsunesada

    TAUP2007: TENTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS   120   2008( ISSN:1742-6588

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    Publishing type:Research paper (international conference proceedings)  

    We present in the results of TAMA300 data analysis for short duration gravitational waves. The excess power filter, alternative linear filter (ALF) and TF(time-frequency) clustering methods have been employed for burst gravitational waves from stellar-core collapse, and matched filtering method used for the ringdown gravitational waves from black hole quasi-normal oscillations. The observational range of TAMA for the burst gravitational waves is roughly 1 kpc, and the range for black hole ringdown covers most of our galaxy. We have been developed new method 'time-frequency (TF) clustering' to find the burst waves. This is a TF clustering method on spectrogram (sonogram). Using this method, we can efficiently identify some predicted gravitational wave forms[2] and can exclude typical unstable spike like noises.

    DOI: 10.1088/1742-6596/120/3/032013

  • Search for continuous gravitational waves from PSR J0835-4510 using CLIO data Reviewed

    Akutsu Tomomi, Ando Masaki, Haruyama Tomiyoshi, Kanda Nobuyuki, Kuroda Kazuaki, Miyoki Sinji, Ohashi Masatake, Saito Yoshio, Sato Nobuaki, Shintomi Takakazu, Suzuki Toshikazu, Tagoshi Hideyuki, Takahashi Hirotaka, Tatsumi Daisuke, Telada Souichi, Tomaru Takayuki, Uchiyama Takashi, Yamamoto Akira, Yamamoto Kazuhiro

    Classical and Quantum Gravity   25 ( 18 )   184013 - 184013   2008( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/0264-9381/25/18/184013

    Other URL: http://orcid.org/0000-0002-8865-9998

  • DECIGO Pathfinder Reviewed

    Ando Masaki, Kawamura Seiji, Nakamura Takashi, Tsubono Kimio, Tanaka Takahiro, Funaki Ikkoh, Seto Naoki, Numata Kenji, Sato Shuichia, Ioka Kunihito, Kanda Nobuyuki, Takashima Takeshi, Agatsuma Kazuhiro, Akutsu Tomotada, Akutsu Tomomi, Aoyanagi Koh-suke, Arai Koji, Arase Yuta, Araya Akito, Asada Hideki, Aso Yoichi, Chiba Takeshi, Ebisuzaki Toshikazu, Enoki Motohiro, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Ganzu Katsuhiko, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Hong Feng-Lei, Horisawa Hideyuki, Hosokawa Mizuhiko, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T, Ishidoshiro Koji, Ishihara Hideki, Ishikawa Takehiko, Ishizaki Hideharu, Ito Hiroyuki, Itoh Yousuke, Kamagasako Shogo, Kawashima Nobuki, Kawazoe Fumiko, Kirihara Hiroyuki, Kishimoto Naoko, Kiuche Kenta, Kobayashi Shiho, Kohri Kazunori, Koizumi Hiroyuki, Kojima Yasufumi, Kokeyama Keiko, Kokuyama Wataru, Kotake Kei, Kozai Yoshihide, Kudoh Hideaki, Kunimori Hiroo, Kuninaka Hitoshi, Kuroda Kazuaki, Maeda Kei-ichi, Matsuhara Hideo, Mino Yasushi, Miyakawa Osamu, Miyoki Shinji, Morimoto Mutsuko Y, Morioka Tomoko, Morisawa Toshiyuki, Moriwaki Shigenori, Mukohyama Shinji, Musha Mitsuru, Nagano Shigeo, Naito Isao, Nakagawa Noriyasu, Nakamura Kouji, Nakano Hiroyuki, Nakao Kenichi, Nakasuka Shinichi, Nakayama Yoshinori, Nishida Erina, Nishiyama Kazutaka, Nishizawa Atsushi, Niwa Yoshito, Ohashi Masatake, Ohishi Naoko, Ohkawa Masashi, Okutomi Akira, Onozato Kouji, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Sakagami Masaaki, Sakai Shin-ichiro, Sakata Shihori, Sasaki Misao, Sato Takashi, Shibata Masaru, Shinkai Hisaaki, Somiya Kentaro, Sotani Hajime, Sugiyama Naoshi, Suwa Yudai, Tagoshi Hideyuki, Takahashi Kakeru, Takahashi Keitaro, Takahashi Tadayuki, Takahashi Hirotaka, Takahashi Ryuichi, Takahashi Ryutaro, Takamori Akiteru, Takano Tadashi, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Tokuda Mitsuru, Tokunari Masao, Toyoshima Morio, Tsujikawa Shinji, Tsunesada Yoshiki, Ueda Ken-ichi, Utashima Masayoshi, Yamakawa Hiroshi, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yokoyama Jun'ichi, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh

    TAUP2007: TENTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS   120   2008( ISSN:1742-6588

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    DOI: 10.1088/1742-6596/120/3/032005

  • A systematical veto by all monitor signals in a gravitational-wave detector Reviewed

    Ishidoshiro Koji, Ando Masaki, Tsubono Kimio, Kanda Nobuyuki, Takahashi Hirotaka

    CLASSICAL AND QUANTUM GRAVITY   24 ( 19 )   S405 - S413   2007.10( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/24/19/S04

  • Current status of Japanese detectors Reviewed

    Tatsumi Daisuke, Takahashi Ryutaro, Arai Koji, Nakagawa Noriyasu, Agatsuma Kazuhiro, Yamazaki Toshitaka, Fukushima Mitsuhiro, Fujimoto Masa-Katsu, Takamori Akiteru, Bertolini Alessandro, Sannibale Virginio, DeSalvo Riccardo, Marka Szabolcs, Ando Masaki, Tsubono Kimio, Akutsu Tomomi, Yamamoto Kazuhiro, Ishitsuka Hideki, Uchiyama Takashi, Miyoki Shinji, Ohashi Masatake, Kuroda Kazuaki, Awaya Norichika, Kanda Nobuyuki, Araya Akito, Telada Souichi, Tomaru Takayuki, Haruyama Tomiyoshi, Yamamoto Akira, Sato Nobuaki, Suzuki Toshitaka, Shintomi Takakazu

    CLASSICAL AND QUANTUM GRAVITY   24 ( 19 )   S399 - S403   2007.10( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/24/19/S03

  • Detecting gravitational waves from inspiraling binaries with a network of detectors: Coherent strategies for correlated detectors Reviewed

    Tagoshi Hideyuki, Mukhopadhyay Himan, Dhurandhar Sanjeev, Sago Norichika, Takahashi Hirotaka, Kanda Nobuyuki

    PHYSICAL REVIEW D   75 ( 8 )   2007.04( ISSN:1550-7998

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    DOI: 10.1103/PhysRevD.75.087306

  • Detecting gravitational waves from inspiraling binaries with a network of detectors: Coherent strategies for correlated detectors Reviewed

    Hideyuki Tagoshi, Himan Mukhopadhyay, Sanjeev Dhurandhar, Norichika Sago, Hirotaka Takahashi, Nobuyuki Kanda

    PHYSICAL REVIEW D   75 ( 8 )   2007.04( ISSN:1550-7998

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    We discuss the coherent search strategy to detect gravitational waves from inspiraling compact binaries by a network of correlated laser interferometric detectors. From the maximum likelihood ratio statistic, we obtain a coherent statistic which is slightly different from and generally better than what we obtained in our previous work. In the special case when the cross spectrum of two detectors normalized by the power spectrum density is constant, the new statistic agrees with the old one. The quantitative difference of the detection probability for a given false alarm rate is also evaluated in a simple case.

    DOI: 10.1103/PhysRevD.75.087306

  • 21pZH-2 Status of development for interferometric gravitational wave detector TAMA300 XV : Seismic Attenuation System 2 Reviewed

    Agatsuma K., Takamori A., Bertolini A., DeSalvo R., Sato S., Aso Y., Akutsu T., Tsunesada Y., Nagano S., Ando M., Miyoki S., Takahashi R., Moriwaki S., Kanda N., Musha M., Fujimoto M.-K., Kawamura S., Mio N., Ohashi M., Kuroda K., Tsubono K., TAMA Collaboration, Arase Y., Hukushima M., Yamazaki T., Ishizaki H., Arai K., Tatsumi D., Izumi K.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   62 ( 0 )   2007

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    DOI: 10.11316/jpsgaiyo.62.2.1.0_99_2

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  • 28pSG-5 The effect of the cosmic rays on the interferometeric gravitational wave detector Reviewed

    Yamamoto K., Tsunesada Y., Okada A., Uchiyama T., Miyoki S., Ohashi M., Kuroda K., Hayakawa H., Kanda N., Tatsumi D.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   62 ( 0 )   2007

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    DOI: 10.11316/jpsgaiyo.62.1.1.0_113_4

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  • 27pSG-6 Status of Development for Interferometric Gravitational Wave Detector TAMA300 XIII : Interferometer Development Reviewed

    Arai K., Bertolini A., DeSalvo R., Sato S., Aso Y., Akutsu T., Tsunesada Y., Nagano S., Ando M., Miyoki S., Moriwaki S., Tatsumi D., Kanda N., Musha M., Fujimoto M.-K., Kawamura S., Mio N., Ohashi M., Kuroda K., Tsubono K., TAMA Collaboration, Takahashi R., Nakagawa N., Agatsuma K., Arase Y., Fukushima M., Yamazaki T., Takamori A.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   62 ( 0 )   2007

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    DOI: 10.11316/jpsgaiyo.62.1.1.0_109_2

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  • 21pZH-5 Status of Development for Interferometric Gravitational Wave Detector TAMA300 XVIII : Interferometer Development Reviewed

    Arai K., Takamori A., Bertolini A., DeSalvo R., Sato S., Aso Y., Akutsu T., Tsunesada Y., Nagano S., Ando M., Miyoki S., Tatsumi D., Moriwaki S., Kanda N., Musha M., Fujimoto M.-K., Kawamura S., Mio N., Ohashi M., Kuroda K., Tsubono K., TAMA Collaboration, Izumi K., Takahashi R., Agatsuma K., Arase Y., Fukushima M., Yamazaki T., Ishizaki H.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   62 ( 0 )   2007

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    DOI: 10.11316/jpsgaiyo.62.2.1.0_100_1

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  • 21pZH-5 干渉計型重力波検出器TAMA300開発の現状 XVIII : 干渉計開発(21pZH 重力波,宇宙線・宇宙物理領域) Reviewed

    新井 宏二, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 辰巳 大輔, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 和泉 究, 高橋 竜太郎, 我妻 一博, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴

    一般社団法人 日本物理学会 日本物理学会講演概要集   62 ( 0 )   100 - 100   2007( ISSN:1342-8349 ( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.62.2.1.0_100_1

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  • Current status of Japanese detectors. Reviewed

    Daisuke Tatsumi, Ryutaro Takahashi, Koji Arai, Noriyasu Nakagawa, Kazuhiro Agatsuma, Toshitaka Yamazaki, Mitsuhiro Fukushima, Masa-Katsu Fujimoto, Akiteru Takamori, Alessandro Bertolini, Virginio Sannibale, Riccardo DeSalvo, Szabolcs Marka, Masaki Ando, Kimio Tsubono, Tomomi Akutsu, Kazuhiro Yamamoto, Hideki Ishitsuka, Takashi Uchiyama, Shinji Miyoki, Masatake Ohashi, Kazuaki Kuroda, Norichika Awaya, Nobuyuki Kanda, Akito Araya, Souichi Telada, Takayuki Tomaru, Tomiyoshi Haruyama, Akira Yamamoto, Nobuaki Sato, Toshitaka Suzuki, Takakazu Shintomi

    Classical and Quantum Gravity   24 ( 19 )   S399 - S403   2007( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/0264-9381/24/19/S03

  • A systematical veto by all monitor signals in a gravitational-wave detector Reviewed

    Ishidoshiro Koji, Ando Masaki, Tsubono Kimio, Kanda Nobuyuki, Takahashi Hirotaka, TAMA Collaboration

    Classical and Quantum Gravity   24 ( 19 )   S405 - S413   2007( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/0264-9381/24/19/S04

    Other URL: http://orcid.org/0000-0002-8865-9998

  • 28pSG-5 The effect of the cosmic rays on the interferometeric gravitational wave detector

    Yamamoto K., Okada A., Uchiyama T., Miyoki S., Ohashi M., Kuroda K., Hayakawa H., Kanda N., Tatsumi D., Tsunesada Y.

    Meeting Abstracts of the Physical Society of Japan   62.1.1 ( 0 )   113   2007( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.62.1.1.0_113_4

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  • 27pSG-6 干渉計型重力波検出器TAMA300開発の現状XIII : 干渉計開発(27pSG 重力波,宇宙線・宇宙物理領域) Reviewed

    新井 宏二, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 森脇 成典, 辰巳 大輔, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 高橋 竜太郎, 中川 憲保, 我妻 一博, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 高森 昭光

    一般社団法人 日本物理学会 日本物理学会講演概要集   62 ( 0 )   109 - 109   2007( ISSN:1342-8349 ( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.62.1.1.0_109_2

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  • Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004 Reviewed

    Akutsu Tomomi, Akutsu Tomotada, Ando Masaki, Arai Koji, Araya Akito, Asada Hideki, Aso Youichi, Barton Mark A., Beyersdorf Peter, Fujiki Youhei, Fujimoto Masa-Katsu, Fujita Ryuichi, Fukushima Mitsuhiro, Futamase Toshifumi, Hamuro Yusaku, Haruyama Tomiyoshi, Hayakawa Hideaki, Hayama Kazuhiro, Heinzel Gerhard, Horikoshi Gen'ichi, Iguchi Hideo, Iida Yukiyoshi, Ioka Kunihito, Ishitsuka Hideki, Kamikubota Norihiko, Kanda Nobuyuki, Kaneyama Takaharu, Karasawa Yoshikazu, Kasahara Kunihiko, Kasai Taketoshi, Katsuki Mayu, Kawabe Keita, Kawamura Mari, Kawamura Seiji, Kawashima Nobuki, Kawazoe Fumiko, Kojima Yasufumi, Kokeyama Keiko, Kondo Kazuhiro, Kozai Yoshihide, Kudoh Hideaki, Kuroda Kazuaki, Kuwabara Takashi, Matsuda Namio, Mio Norikatsu, Miura Kazuyuki, Miyakawa Osamu, Miyama Shoken, Miyoki Shinji, Mizusawa Hiromi, Moriwaki Shigenori, Musha Mitsuru, Nagano Shigeo, Nagayama Yoshitaka, Nakagawa Ken'ichi, Nakamura Takashi, Nakano Hiroyuki, Nakao Ken-ichi, Nishi Yuhiko, Numata Kenji, Ogawa Yujiro, Ohashi Masatake, Ohishi Naoko, Okutomi Akira, Oohara Ken-ichi, Otsuka Shigemi, Sago Norichika, Saito Yoshio, Sakata Shihori, Sasaki Misao, Sato Kouichi, Sato Nobuaki, Sato Shuichi, Sato Youhei, Seki Hidetsugu, Sekido Aya, Seto Naoki, Shibata Masaru, Shinkai Hisaaki, Shintomi Takakazu, Soida Kenji, Somiya Kentaro, Suzuki Toshikazu, Tagoshi Hideyuki, Takahashi Hirotaka, Takahashi Ryutaro, Takamori Akiteru, Takemoto Shuzo, Takeno Kohei, Tanaka Takahiro, Taniguchi Keisuke, Taniguchi Shinsuke, Tanji Toru, Tatsumi Daisuke, Taylor C. T., Telada Souichi, Tochikubo Kuniharu, Tokunari Masao, Tomaru Takayuki, Tsubono Kimio, Tsuda Nobuhiro, Tsunesada Yoshiki, Uchiyama Takashi, Ueda Akitoshi, Ueda Ken-ichi, Usui Fumihiko, Waseda Koichi, Watanabe Yuko, Yakura Hiromi, Yamamoto Akira, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yanagi Yuriko, Yoda Tatsuo, Yokoyama Jun'ichi, Yoshida Tatsuru, Zhu Zong-Hong

    PHYSICAL REVIEW D   74 ( 12 )   2006.12( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.74.122002

  • Analysis of gravitational wave bursts in TAMA300 data using an ALF filter Reviewed

    Akutsu T., Ando M., Kanda N., Tatsumi D., Telada S., Miyoki S., Ohashi M.

    CLASSICAL AND QUANTUM GRAVITY   23 ( 19 )   S715 - S721   2006.10( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/23/19/S10

  • Detecting gravitational waves from inspiraling binaries with a network of detectors: Coherent versus coincident strategies Reviewed

    Mukhopadhyay Himan, Sago Norichika, Tagoshi Hideyuki, Dhurandhar Sanjeev, Takahashi Hirotaka, Kanda Nobuyuki

    PHYSICAL REVIEW D   74 ( 8 )   2006.10( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.74.083005

  • Detecting gravitational waves from inspiraling binaries with a network of detectors: Coherent versus coincident strategies Reviewed

    Himan Mukhopadhyay, Norichika Sago, Hideyuki Tagoshi, Sanjeev Dhurandhar, Hirotaka Takahashi, Nobuyuki Kanda

    PHYSICAL REVIEW D   74 ( 8 )   2006.10( ISSN:2470-0010 ( eISSN:2470-0029

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    We compare two strategies of multidetector detection of compact binary inspiral signals, namely, the coincidence and the coherent. For simplicity we consider here two identical detectors having the same power spectral density of noise, that of initial LIGO, located in the same place and having the same orientation. We consider the cases of independent noise as well as that of correlated noise. The coincident strategy involves separately making two candidate event lists, one for each detector, and from these choosing those pairs of events from the two lists which lie within a suitable parameter window, which then are called coincidence detections. The coherent strategy on the other hand involves combining the data phase coherently, so as to obtain a single network statistic which is then compared with a single threshold. Here we attempt to shed light on the question as to which strategy is better. We compare the performances of the two methods by plotting the receiver operating characteristics (ROC) for the two strategies. Several of the results are obtained analytically in order to gain insight. Further we perform numerical simulations in order to determine certain parameters in the analytic formulae and thus obtain the final complete results. We consider here several cases from the relatively simple to the astrophysically more relevant in order to establish our results. The bottom line is that the coherent strategy although more computationally expensive in general than the coincidence strategy, is superior to the coincidence strategy-considerably less false dismissal probability for the same false alarm probability in the viable false alarm regime.

    DOI: 10.1103/PhysRevD.74.083005

  • Experimental Efforts to Detect Gravitational Waves : Large Scale Cryogenic Gravitational Wave Telscope Reviewed

    Kuroda Kazuaki, Kanda Nobuyuki, Ohashi Masatake, SAITO Yoshio, TAKAHASHI Ryutaro, ANDO Masaki, MIO Norikatsu, TELADA Soichi, MORIWAKI Shigenori, UCHIYAMA Takashi, TOMARU Takayuki, SUZUKI Toshikazu, MIYOKI Shinji, TAKAMORI Akiteru, TATSUMI Daisuke, COLLABORATION LCGT

    Published for the Yukawa Institute for Theoretical Physics and the Physical Society of Japan Progress of theoretical physics. Supplement   ( 163 )   54 - 99   2006.07( ISSN:03759687

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    A remarkable design of LCGT was established by experimental efforts to detect gravitational waves in Japan including optional alternatives in design detail. The LCGT adopts an advanced technique regarded to be used in the third generation. We can reliably detect gravitational waves by LCGT and still have a chance to firstly detect it.

    DOI: 10.1143/PTPS.163.54

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  • Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries Reviewed

    Abbott B., Abbott R., Adhikari R., Ageev A., Agresti J., Ajith P., Allen B., Allen J., Amin R., Anderson S. B., Anderson W. G., Araya M., Armandula H., Ashley M., Asiri F., Aufmuth P., Aulbert C., Babak S., Balasubramanian R., Ballmer S., Barish B. C., Barker C., Barker D., Barnes M., Barr B., Barton M. A., Bayer K., Beausoleil R., Belczynski K., Bennett R., Berukoff S. J., Betzwieser J., Bhawal B., Bilenko I. A., Billingsley G., Black E., Blackburn K., Blackburn L., Bland B., Bochner B., Bogue L., Bork R., Bose S., Brady P. R., Braginsky V. B., Brau J. E., Brown D. A., Bullington A., Bunkowski A., Buonanno A., Burgess R., Busby D., Butler W. E., Byer R. L., Cadonati L., Cagnoli G., Camp J. B., Cannizzo J., Cannon K., Cantley C. A., Cao J., Cardenas L., Carter K., Casey M. M., Castiglione J., Chandler A., Chapsky J., Charlton P., Chatterji S., Chelkowski S., Chen Y., Chickarmane V., Chin D., Christensen N., Churches D., Cokelaer T., Colacino C., Coldwell R., Coles M., Cook D., Corbitt T., Coyne D., Creighton J. D. E., Creighton T. D., Crooks D. R. M., Csatorday P., Cusack B. J., Cutler C., Dalrymple J., D'Ambrosio E., Danzmann K., Davies G., Daw E., DeBra D., Delker T., Dergachev V., Desai S., DeSalvo R., Dhurandhar S., Di Credico A., Diaz M., Ding H., Drever R. W. P., Dupuis R. J., Edlund J. A., Ehrens P., Elliffe E. J., Etzel T., Evans M., Evans T., Fairhurst S., Fallnich C., Farnham D., Fejer M. M., Findley T., Fine M., Finn L. S., Franzen K. Y., Freise A., Frey R., Fritschel P., Frolov V. V., Fyffe M., Ganezer K. S., Garofoli J., Giaime J. A., Gillespie A., Goda K., Goggin L., Gonzalez G., Gossler S., Grandclement P., Grant A., Gray C., Gretarsson A. M., Grimmett D., Grote H., Grunewald S., Guenther M., Gustafson E., Gustafson R., Hamilton W. O., Hammond M., Hanna C., Hanson J., Hardham C., Harms J., Harry G., Hartunian A., Heefner J., Hefetz Y., Heinzel G., Heng I. S., Hennessy M., Hepler N., Heptonstall A., Heurs M., Hewitson M., Hild S., Hindman N., Hoang P., Hough J., Hrynevych M., Hua W., Ito M., Itoh Y., Ivanov A., Jennrich O., Johnson B., Johnson W. W., Johnston W. R., Jones D. I., Jones G., Jones L., Jungwirth D., Kalogera V., Katsavounidis E., Kawabe K., Kells W., Kern J., Khan A., Killbourn S., Killow C. J., Kim C., King C., King P., Klimenko S., Koranda S., Koetter K., Kovalik J., Kozak D., Krishnan B., Landry M., Langdale J., Lantz B., Lawrence R., Lazzarini A., Lei M., Leonor I., Libbrecht K., Libson A., Lindquist P., Liu S., Logan J., Lormand M., Lubinski M., Lueck H., Luna M., Lyons T. T., Machenschalk B., MacInnis M., Mageswaran M., Mailand K., Majid W., Malec M., Mandic V., Mann F., Marin A., Marka S., Maros E., Mason J., Mason K., Matherny O., Matone L., Mavalvala N., McCarthy R., McClelland D. E., McHugh M., McNabb J. W. C., Melissinos A., Mendell G., Mercer R. A., Meshkov S., Messaritaki E., Messenger C., Mikhailov E., Mitra S., Mitrofanov V. P., Mitselmakher G., Mittleman R., Miyakawa O., Mohanty S., Moreno G., Mossavi K., Mueller G., Mukherjee S., Murray P., Myers E., Myers J., Nagano S., Nash T., Nayak R., Newton G., Nocera F., Noel J. S., Nutzman P., Olson T., O'Reilly B., Ottaway D. J., Ottewill A., Ouimette D., Overmier H., Owen B. J., Pan Y., Papa M. A., Parameshwaraiah V., Parameswariah C., Pedraza M., Penn S., Pitkin M., Plissi M., Prix R., Quetschke V., Raab F., Radkins H., Rahkola R., Rakhmanov M., Rao S. R., Rawlins K., Ray-Majumder S., Re V., Redding D., Regehr M. W., Regimbau T., Reid S., Reilly K. T., Reithmaier K., Reitze D. H., Richman S., Riesen R., Riles K., Rivera B., Rizzi A., Robertson D. I., Robertson N. A., Robinson C., Robison L., Roddy S., Rodriguez A., Rollins J., Romano J. D., Romie J., Rong H., Rose D., Rotthoff E., Rowan S., Ruediger A., Ruet L., Russell P., Ryan K., Salzman I., Sandberg V., Sanders G. H., Sannibale V., Sarin P., Sathyaprakash B., Saulson P. R., Savage R., Sazonov A., Schilling R., Schlaufman K., Schmidt V., Schnabel R., Schofield R., Schutz B. F., Schwinberg P., Scott S. M., Seader S. E., Searle A. C., Sears B., Seel S., Seifert F., Sellers D., Sengupta A. S., Shapiro C. A., Shawhan P., Shoemaker D. H., Shu Q. Z., Sibley A., Siemens X., Sievers L., Sigg D., Sintes A. M., Smith J. R., Smith M., Smith M. R., Sneddon P. H., Spero R., Spjeld O., Stapfer G., Steussy D., Strain K. A., Strom D., Stuver A., Summerscales T., Sumner M. C., Sung M., Sutton P. J., Sylvestre J., Tanner D. B., Tariq H., Tarallo M., Taylor I., Taylor R., Taylor R., Thorne K. A., Thorne K. S., Tibbits M., Tilav S., Tinto M., Tokmakov K. V., Torres C., Torrie C., Traylor G., Tyler W., Ugolini D., Ungarelli C., Vallisneri M., van Putten M., Vass S., Vecchio A., Veitch J., Vorvick C., Vyachanin S. P., Wallace L., Walther H., Ward H., Ward R., Ware B., Watts K., Webber D., Weidner A., Weiland U., Weinstein A., Weiss R., Welling H., Wen L., Wen S., Wette K., Whelan J. T., Whitcomb S. E., Whiting B. F., Wiley S., Wilkinson C., Willems P. A., Williams P. R., Williams R., Willke B., Wilson A., Winjum B. J., Winkler W., Wise S., Wiseman A. G., Woan G., Woods D., Wooley R., Worden J., Wu W., Yakushin I., Yamamoto H., Yoshida S., Zaleski K. D., Zanolin M., Zawischa I., Zhang L., Zhu R., Zotov N., Zucker M., Zweizig J., Akutsu T., Akutsu T., Ando M., Arai K., Araya A., Asada H., Aso Y., Beyersdorf P., Fujiki Y., Fujimoto M. -K., Fujita R., Fukushima M., Futamase T., Hamuro Y., Haruyama T., Hayama K., Iguchi H., Iida Y., Ioka K., Ishitsuka H., Kamikubota N., Kanda N., Kaneyama T., Karasawa Y., Kasahara K., Kasai T., Katsuki M., Kawamura S., Kawamura M., Kawazoe F., Kojima Y., Kokeyama K., Kondo K., Kozai Y., Kudoh H., Kuroda K., Kuwabara T., Matsuda N., Mio N., Miura K., Miyama S., Miyoki S., Mizusawa H., Moriwaki S., Musha M., Nagayama Y., Nakagawa K., Nakamura T., Nakano H., Nakao K., Nishi Y., Numata K., Ogawa Y., Ohashi M., Ohishi N., Okutomi A., Oohara K., Otsuka S., Saito Y., Sakata S., Sasaki M., Sato N., Sato S., Sato Y., Sato K., Sekido A., Seto N., Shibata M., Shinkai H., Shintomi T., Soida K., Somiya K., Suzuki T., Tagoshi H., Takahashi H., Takahashi R., Takamori A., Takemoto S., Takeno K., Tanaka T., Taniguchi K., Tanji T., Tatsumi D., Telada S., Tokunari M., Tomaru T., Tsubono K., Tsuda N., Tsunesada Y., Uchiyama T., Ueda K., Ueda A., Waseda K., Yamamoto A., Yamamoto K., Yamazaki T., Yanagi Y., Yokoyama J., Yoshida T., Zhu Z. -H.

    PHYSICAL REVIEW D   73 ( 10 )   2006.05( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.73.102002

  • Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries Reviewed

    B. Abbott, R. Abbott, R. Adhikari, A. Ageev, J. Agresti, P. Ajith, B. Allen, J. Allen, R. Amin, S. B. Anderson, W. G. Anderson, M. Araya, H. Armandula, M. Ashley, F. Asiri, P. Aufmuth, C. Aulbert, S. Babak, R. Balasubramanian, S. Ballmer, B. C. Barish, C. Barker, D. Barker, M. Barnes, B. Barr, M. A. Barton, K. Bayer, R. Beausoleil, K. Belczynski, R. Bennett, S. J. Berukoff, J. Betzwieser, B. Bhawal, I. A. Bilenko, G. Billingsley, E. Black, K. Blackburn, L. Blackburn, B. Bland, B. Bochner, L. Bogue, R. Bork, S. Bose, P. R. Brady, V. B. Braginsky, J. E. Brau, D. A. Brown, A. Bullington, A. Bunkowski, A. Buonanno, R. Burgess, D. Busby, W. E. Butler, R. L. Byer, L. Cadonati, G. Cagnoli, J. B. Camp, J. Cannizzo, K. Cannon, C. A. Cantley, J. Cao, L. Cardenas, K. Carter, M. M. Casey, J. Castiglione, A. Chandler, J. Chapsky, P. Charlton, S. Chatterji, S. Chelkowski, Y. Chen, V. Chickarmane, D. Chin, N. Christensen, D. Churches, T. Cokelaer, C. Colacino, R. Coldwell, M. Coles, D. Cook, T. Corbitt, D. Coyne, J. D. E. Creighton, T. D. Creighton, D. R. M. Crooks, P. Csatorday, B. J. Cusack, C. Cutler, J. Dalrymple, E. D'Ambrosio, K. Danzmann, G. Davies, E. Daw, D. DeBra, T. Delker, V. Dergachev, S. Desai, R. DeSalvo, S. Dhurandhar, A. Di Credico, M. Diaz, H. Ding, R. W. P. Drever, R. J. Dupuis, J. A. Edlund, P. Ehrens, E. J. Elliffe, T. Etzel, M. Evans, T. Evans, S. Fairhurst, C. Fallnich, D. Farnham, M. M. Fejer, T. Findley, M. Fine, L. S. Finn, K. Y. Franzen, A. Freise, R. Frey, P. Fritschel, V. V. Frolov, M. Fyffe, K. S. Ganezer, J. Garofoli, J. A. Giaime, A. Gillespie, K. Goda, L. Goggin, G. Gonzalez, S. Gossler, P. Grandclement, A. Grant, C. Gray, A. M. Gretarsson, D. Grimmett, H. Grote, S. Grunewald, M. Guenther, E. Gustafson, R. Gustafson, W. O. Hamilton, M. Hammond, C. Hanna, J. Hanson, C. Hardham, J. Harms, G. Harry, A. Hartunian, J. Heefner, Y. Hefetz, G. Heinzel, I. S. Heng, M. Hennessy, N. Hepler, A. Heptonstall, M. Heurs, M. Hewitson, S. Hild, N. Hindman, P. Hoang, J. Hough, M. Hrynevych, W. Hua, M. Ito, Y. Itoh, A. Ivanov, O. Jennrich, B. Johnson, W. W. Johnson, W. R. Johnston, D. I. Jones, G. Jones, L. Jones, D. Jungwirth, V. Kalogera, E. Katsavounidis, K. Kawabe, W. Kells, J. Kern, A. Khan, S. Killbourn, C. J. Killow, C. Kim, C. King, P. King, S. Klimenko, S. Koranda, K. Koetter, J. Kovalik, D. Kozak, B. Krishnan, M. Landry, J. Langdale, B. Lantz, R. Lawrence, A. Lazzarini, M. Lei, I. Leonor, K. Libbrecht, A. Libson, P. Lindquist, S. Liu, J. Logan, M. Lormand, M. Lubinski, H. Lueck, M. Luna, T. T. Lyons, B. Machenschalk, M. MacInnis, M. Mageswaran, K. Mailand, W. Majid, M. Malec, V. Mandic, F. Mann, A. Marin, S. Marka, E. Maros, J. Mason, K. Mason, O. Matherny, L. Matone, N. Mavalvala, R. McCarthy, D. E. McClelland, M. McHugh, J. W. C. McNabb, A. Melissinos, G. Mendell, R. A. Mercer, S. Meshkov, E. Messaritaki, C. Messenger, E. Mikhailov, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, S. Mohanty, G. Moreno, K. Mossavi, G. Mueller, S. Mukherjee, P. Murray, E. Myers, J. Myers, S. Nagano, T. Nash, R. Nayak, G. Newton, F. Nocera, J. S. Noel, P. Nutzman, T. Olson, B. O'Reilly, D. J. Ottaway, A. Ottewill, D. Ouimette, H. Overmier, B. J. Owen, Y. Pan, M. A. Papa, V. Parameshwaraiah, C. Parameswariah, M. Pedraza, S. Penn, M. Pitkin, M. Plissi, R. Prix, V. Quetschke, F. Raab, H. Radkins, R. Rahkola, M. Rakhmanov, S. R. Rao, K. Rawlins, S. Ray-Majumder, V. Re, D. Redding, M. W. Regehr, T. Regimbau, S. Reid, K. T. Reilly, K. Reithmaier, D. H. Reitze, S. Richman, R. Riesen, K. Riles, B. Rivera, A. Rizzi, D. I. Robertson, N. A. Robertson, C. Robinson, L. Robison, S. Roddy, A. Rodriguez, J. Rollins, J. D. Romano, J. Romie, H. Rong, D. Rose, E. Rotthoff, S. Rowan, A. Ruediger, L. Ruet, P. Russell, K. Ryan, I. Salzman, V. Sandberg, G. H. Sanders, V. Sannibale, P. Sarin, B. Sathyaprakash, P. R. Saulson, R. Savage, A. Sazonov, R. Schilling, K. Schlaufman, V. Schmidt, R. Schnabel, R. Schofield, B. F. Schutz, P. Schwinberg, S. M. Scott, S. E. Seader, A. C. Searle, B. Sears, S. Seel, F. Seifert, D. Sellers, A. S. Sengupta, C. A. Shapiro, P. Shawhan, D. H. Shoemaker, Q. Z. Shu, A. Sibley, X. Siemens, L. Sievers, D. Sigg, A. M. Sintes, J. R. Smith, M. Smith, M. R. Smith, P. H. Sneddon, R. Spero, O. Spjeld, G. Stapfer, D. Steussy, K. A. Strain, D. Strom, A. Stuver, T. Summerscales, M. C. Sumner, M. Sung, P. J. Sutton, J. Sylvestre, D. B. Tanner, H. Tariq, M. Tarallo, I. Taylor, R. Taylor, R. Taylor, K. A. Thorne, K. S. Thorne, M. Tibbits, S. Tilav, M. Tinto, K. V. Tokmakov, C. Torres, C. Torrie, G. Traylor, W. Tyler, D. Ugolini, C. Ungarelli, M. Vallisneri, M. van Putten, S. Vass, A. Vecchio, J. Veitch, C. Vorvick, S. P. Vyachanin, L. Wallace, H. Walther, H. Ward, R. Ward, B. Ware, K. Watts, D. Webber, A. Weidner, U. Weiland, A. Weinstein, R. Weiss, H. Welling, L. Wen, S. Wen, K. Wette, J. T. Whelan, S. E. Whitcomb, B. F. Whiting, S. Wiley, C. Wilkinson, P. A. Willems, P. R. Williams, R. Williams, B. Willke, A. Wilson, B. J. Winjum, W. Winkler, S. Wise, A. G. Wiseman, G. Woan, D. Woods, R. Wooley, J. Worden, W. Wu, I. Yakushin, H. Yamamoto, S. Yoshida, K. D. Zaleski, M. Zanolin, I. Zawischa, L. Zhang, R. Zhu, N. Zotov, M. Zucker, J. Zweizig, T. Akutsu, T. Akutsu, M. Ando, K. Arai, A. Araya, H. Asada, Y. Aso, P. Beyersdorf, Y. Fujiki, M. -K. Fujimoto, R. Fujita, M. Fukushima, T. Futamase, Y. Hamuro, T. Haruyama, K. Hayama, H. Iguchi, Y. Iida, K. Ioka, H. Ishitsuka, N. Kamikubota, N. Kanda, T. Kaneyama, Y. Karasawa, K. Kasahara, T. Kasai, M. Katsuki, S. Kawamura, M. Kawamura, F. Kawazoe, Y. Kojima, K. Kokeyama, K. Kondo, Y. Kozai, H. Kudoh, K. Kuroda, T. Kuwabara, N. Matsuda, N. Mio, K. Miura, S. Miyama, S. Miyoki, H. Mizusawa, S. Moriwaki, M. Musha, Y. Nagayama, K. Nakagawa, T. Nakamura, H. Nakano, K. Nakao, Y. Nishi, K. Numata, Y. Ogawa, M. Ohashi, N. Ohishi, A. Okutomi, K. Oohara, S. Otsuka, Y. Saito, S. Sakata, M. Sasaki, N. Sato, S. Sato, Y. Sato, K. Sato, A. Sekido, N. Seto, M. Shibata, H. Shinkai, T. Shintomi, K. Soida, K. Somiya, T. Suzuki, H. Tagoshi, H. Takahashi, R. Takahashi, A. Takamori, S. Takemoto, K. Takeno, T. Tanaka, K. Taniguchi, T. Tanji, D. Tatsumi, S. Telada, M. Tokunari, T. Tomaru, K. Tsubono, N. Tsuda, Y. Tsunesada, T. Uchiyama, K. Ueda, A. Ueda, K. Waseda, A. Yamamoto, K. Yamamoto, T. Yamazaki, Y. Yanagi, J. Yokoyama, T. Yoshida, Z. -H. Zhu

    PHYSICAL REVIEW D   73 ( 10 )   2006.05( ISSN:2470-0010 ( eISSN:2470-0029

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    We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an intercollaboration coincidence search during times when TAMA300 and only one of the LIGO sites were operational. We find no evidence of any gravitational wave signals. We place an observational upper limit on the rate of binary neutron star coalescence with component masses between 1 and 3M of 49 per year per Milky Way equivalent galaxy at a 90% confidence level. The methods developed during this search will find application in future network inspiral analyses.

    DOI: 10.1103/PhysRevD.73.102002

  • The Japanese space gravitational wave antenna - DECIGO Reviewed

    Kawamura Seiji, Nakamura Takashi, Ando Masaki, Seto Naoki, Tsubono Kimio, Numata Kenji, Takahashi Ryuichi, Nagano Shigeo, Ishikawa Takehiko, Musha Mitsuru, Ueda Ken-ichi, Sato Takashi, Hosokawa Mizuhiko, Agatsuma Kazuhiro, Akutsu Tomotada, Aoyanagi Koh-suke, Arai Koji, Araya Akito, Asada Hideki, Aso Yoichi, Chiba Takeshi, Ebisuzaki Toshikazu, Eriguchi Yoshiharu, Fujimoto Masa-Katsu, Fukushima Mitsuhiro, Futamase Toshifumi, Ganzu Katsuhiko, Harada Tomohiro, Hashimoto Tatsuaki, Hayama Kazuhiro, Hikida Wataru, Himemoto Yoshiaki, Hirabayashi Hisashi, Hiramatsu Takashi, Ichiki Kiyotomo, Ikegami Takeshi, Inoue Kaiki T., Ioka Kunihito, Ishidoshiro Koji, Itoh Yousuke, Kamagasako Shogo, Kanda Nobuyuki, Kawashima Nobuki, Kirihara Hiroyuki, Kiuchi Kenta, Kobayashi Shiho, Kohri Kazunori, Kojima Yasufumi, Kokeyama Keiko, Kozai Yoshihide, Kudoh Hideaki, Kunimori Hiroo, Kuroda Kazuaki, Maeda Kei-ichi, Matsuhara Hideo, Mino Yasushi, Miyakawa Osamu, Miyoki Shinji, Mizusawa Hiromi, Morisawa Toshiyuki, Mukohyama Shinji, Naito Isao, Nakagawa Noriyasu, Nakamura Kouji, Nakano Hiroyuki, Nishizawa Atsushi, Niwa Yoshito, Nozawa Choetsu, Ohashi Masatake, Ohishi Naoko, Ohkawa Masashi, Okutomi Akira, Oohara Kenichi, Sago Norichika, Saijo Motoyuki, Sakagami Masaaki, Sakata Shihori, Sasaki Misao, Sato Shuichi, Shibata Masaru, Shinkai Hisaaki, Somiya Kentaro, Sotani Hajime, Sugiyama Naoshi, Tagoshi Hideyuki, Takahashi Tadayuki, Takahashi Hirotaka, Takahashi Ryutaro, Takano Tadashi, Tanaka Takahiro, Taniguchi Keisuke, Taruya Atsushi, Tashiro Hiroyuki, Tokunari Masao, Tsujikawa Shinji, Tsunesada Yoshiki, Yamamoto Kazuhiro, Yamazaki Toshitaka, Yokoyama Jun'ichi, Yoo Chul-Moon, Yoshida Shijun, Yoshino Taizoh

    CLASSICAL AND QUANTUM GRAVITY   23 ( 8 )   S125 - S131   2006.04( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/23/8/S17

  • Veto analysis for gravitational wave burst signals in TAMA300 data using an ALF filter Reviewed

    Akutsu T., Ando M., Kanda N., Tatsumi D., Telada S., Miyoki S., Ohashi M.

    CLASSICAL AND QUANTUM GRAVITY   23 ( 8 )   S23 - S28   2006.04( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/23/8/S04

  • 20pSG-2 Status of development for interferometric gravitational wave detector TAMA300 VIII : Seismic Attenuation System Reviewed

    Agatsuma K., Takamori A., Bertolini A., DeSalvo R., Sato S., Akutsu T., Tsunesada Y., Nagano S., Ando M., Miyoki S., Moriwaki S., Takahashi R., Kanda N., Musha M., Fujimoto M.-K., Kawamura S., Mio N., Ohashi M., Kuroda K., Tsubono K., TAMA Collaboration, Arase Y., Tatsumi D., Aso Y., Arai K., Nakagawa N., Hukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   61 ( 0 )   2006

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    DOI: 10.11316/jpsgaiyo.61.2.1.0_56_3

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  • Experimental efforts to detect gravitational waves - Large scale cryogenic gravitational wave telscope Reviewed

    Kuroda Kazuaki, Kanda Nobuyuki, Ohashi Masatake, Saito Yoshio, Takahashi Ryutaro, Ando Masaki, Mio Norikatsu, Telada Soichi, Moriwaki Shigenori, Uchiyama Takashi, Tomaru Takayuki, Suzuki Toshikazu, Miyoki Shinji, Takamori Akiteru, Tatsumi Daisuke, LCGT Collaboration

    Progress of Theoretical Physics Supplement   ( 163 )   54 - 99   2006

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    Other URL: http://orcid.org/0000-0002-8865-9998

  • Experimental efforts to detect gravitational waves - Large scale cryogenic gravitational wave telscope Reviewed

    Kuroda Kazuaki, Kanda Nobuyuki, Ohashi Masatake, Saito Yoshio, Takahashi Ryutaro, Ando Masaki, Mio Norikatsu, Telada Soichi, Moriwaki Shigenori, Uchiyama Takashi, Tomaru Takayuki, Suzuki Toshikazu, Miyoki Shinji, Takamori Akiteru, Tatsumi Daisuke

    PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT   ( 163 )   54 - 99   2006( ISSN:0375-9687

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  • 27aTG-8 Burst GW search with TAMA300 data using multivariate cluster Reviewed

    Honda R, Ando M, Tagoshi H, Tatsumi D, Awaya N, Tokuda M, Kanda N

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   61 ( 0 )   2006

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_86_4

    CiNii Article

  • 27aTG-7 Analysis of TAMA300 data for burst gravitational waves using ALF filter Reviewed

    Akutsu T, Ando M, Kanda N, Tatsumi D, Telada S, Miyoki S, Ohashi M, TAMA Collaboration

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   61 ( 0 )   2006

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_86_3

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  • 27aTG-3 Development status of the interferometric gravitational wave detector TAMA300 VI : Technical elements Reviewed

    Sato S., Takamori A., Iida H., Bertolini A., DeSalvo R., Miyoki S., Nagano S., Ando M., Moriwaki S., Kanda N., Musha M., Arai K., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Ohashi M., Kuroda K., the TAMA Collaboration, Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   61 ( 0 )   2006

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_85_3

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  • 27aTG-2 Status of Development for Interferometric Gravitational Wave Detector TAMA300 V : Interferometer Development Reviewed

    Arai K., Takamori A., Iida H., Bertolini A., DeSalvo R., Miyoki S., Nagano S., Ando M., Moriwaki S., Kanda N., Musha M., Sato S., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Ohashi M., Kuroda K., TAMA Collaboration, Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   61 ( 0 )   2006

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_85_2

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  • 20pSG-5 Evaluation of GCC statistics by using TAMA300 data Reviewed

    ISHIDOSHIRO Koji, HIMEMOTO Yoshiaki, KANDA Nobuyuki, ANDO Masaki, TSUBONO Kimio

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   61 ( 0 )   2006

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    DOI: 10.11316/jpsgaiyo.61.2.1.0_57_1

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  • Results of the search for inspiraling compact star binaries from TAMA300\\'s observation in 2000-2004 Reviewed

    T. Akutsu, T. Akutsu, M. Ando, K. Arai, A. Araya, H. Asada, Y. Aso, M.A. Barton, P. Beyersdorf, Y. Fujiki, M.-K. Fujimoto, R. Fujita, M. Fukushima, T. Futamase, Y. Hamuro, T. Haruyama, H. Hayakawa, K. Hayama, G. Heinzel, G. Horikoshi, H. Iguchi, Y. Iida, K. Ioka, H. Ishitsuka, N. Kamikubota, N. Kanda, T. Kaneyama, Y. Karasawa, K. Kasahara, T. Kasai, M. Katsuki, K. Kawabe, M. Kawamura, S. Kawamura, N. Kawashima, F. Kawazoe, Y. Kojima, K. Kokeyama, K. Kondo, Y. Kozai, H. Kudoh, K. Kuroda, T. Kuwabara, N. Matsuda, N. Mio, K. Miura, O. Miyakawa, S. Miyama, S. Miyoki, H. Mizusawa, S. Moriwaki, M. Musha, S. Nagano, Y. Nagayama, K. Nakagawa, T. Nakamura, H. Nakano, K.-I. Nakao, Y. Nishi, K. Numata, Y. Ogawa, M. Ohashi, N. Ohishi, A. Okutomi, K.-I. Oohara, S. Otsuka, N. Sago, Y. Saito, S. Sakata, M. Sasaki, K. Sato, N. Sato, S. Sato, Y. Sato, H. Seki, A. Sekido, N. Seto, M. Shibata, H. Shinkai, T. Shintomi, K. Soida, K. Somiya, T. Suzuki, H. Tagoshi, H. Takahashi, R. Takahashi, A. Takamori, S. Takemoto, K. Takeno, T. Tanaka, K. Taniguchi, S. Taniguchi, T. Tanji, D. Tatsumi, C.T. Taylor, S. Telada, K. Tochikubo, M. Tokunari, T. Tomaru, K. Tsubono, N. Tsuda, Y. Tsunesada, T. Uchiyama, A. Ueda, K.-I. Ueda, F. Usui, K. Waseda, Y. Watanabe, H. Yakura, A. Yamamoto, K. Yamamoto, T. Yamazaki, Y. Yanagi, T. Yoda, J. Yokoyama, T. Yoshida, Z.-H. Zhu

    Physical Review D - Particles, Fields, Gravitation and Cosmology   74 ( 12 )   2006( ISSN:1550-7998 ( eISSN:1550-2368

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    We analyze the data of the TAMA300 detector to search for gravitational waves from inspiraling compact star binaries with masses of the component stars in the range 1M-3M. In this analysis, 2705 hours of data, taken during the years 2000-2004, are used for the event search. We combine the results of different observation runs, and obtain a single upper limit on the rate of the coalescence of compact binaries in our Galaxy of 20 per year at a 90% confidence level. In this upper limit, the effects of various systematic errors such as the uncertainty of the background estimation and the calibration of the detector's sensitivity are included.

    DOI: 10.1103/PhysRevD.74.122002

  • Analysis of gravitational wave bursts in TAMA300 data using an ALF Filter. Reviewed

    T.Akutsu, M.Ando, N.Kanda, D.Tatsumi, S.Telada, S.Miyoki, M.Ohashi, the TAMA Collaboration

    Classical and Quantum Gravity   23   S715 - S721   2006

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    DOI: 10.1088/0264-9381/23/19/S10

  • 27aTG-8 Burst GW search with TAMA300 data using multivariate cluster

    Honda R, Ando M, Tagoshi H, Tatsumi D, Awaya N, Tokuda M, Kanda N

    Meeting Abstracts of the Physical Society of Japan   61.1.1 ( 0 )   86   2006( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_86_4

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  • 27aTG-7 Analysis of TAMA300 data for burst gravitational waves using ALF filter

    Akutsu T, Ando M, Kanda N, Tatsumi D, Telada S, Miyoki S, Ohashi M, TAMA Collaboration

    Meeting Abstracts of the Physical Society of Japan   61.1.1 ( 0 )   86   2006( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_86_3

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  • 27aTG-3 Development status of the interferometric gravitational wave detector TAMA300 VI : Technical elements

    Sato S., Arai K., Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T., Takamori A., Iida H., Bertolini A., DeSalvo R., Miyoki S., Nagano S., Ando M., Moriwaki S., Kanda N., Musha M., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Ohashi M., Kuroda K., the TAMA Collaboration

    Meeting Abstracts of the Physical Society of Japan   61.1.1 ( 0 )   85   2006( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_85_3

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  • 27aTG-2 干渉計型重力波検出器TAMA300開発の現状V : 干渉計開発(27aTG 重力波,宇宙線・宇宙物理領域) Reviewed

    新井 宏二, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 佐藤 修一, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正健, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   61 ( 0 )   85 - 85   2006( ISSN:1342-8349 ( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.61.1.1.0_85_2

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  • 20pSG-5 Evaluation of GCC statistics by using TAMA300 data

    ISHIDOSHIRO Koji, HIMEMOTO Yoshiaki, KANDA Nobuyuki, ANDO Masaki, TSUBONO Kimio

    Meeting Abstracts of the Physical Society of Japan   61.2.1 ( 0 )   57   2006( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.61.2.1.0_57_1

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  • 20pSG-2 干渉計型重力波検出器TAMA300開発の現状VIII : 低周波防振装置(20pSG 重力波,宇宙線・宇宙物理領域) Reviewed

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 森脇 成典, 高橋 竜太郎, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 辰巳 大輔, 麻生 洋一, 新井 宏二, 中川 憲保, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   61 ( 0 )   56 - 56   2006( ISSN:1342-8349 ( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.61.2.1.0_56_3

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  • Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts Reviewed

    Abbott B, Abbott R, Adhikari R, Ageev A, Agresti J, Ajith P, Allen B, Allen J, Amin R, Anderson SB, Anderson WG, Araya M, Armandula H, Ashley M, Asiri F, Aufmuth P, Aulbert C, Babak S, Balasubramanian R, Ballmer S, Barish BC, Barker C, Barker D, Barnes M, Barr B, Barton MA, Bayer K, Beausoleil R, Belczynski K, Bennett R, Berukoff SJ, Betzwieser J, Bhawal B, Bilenko IA, Billingsley G, Black E, Blackburn K, Blackburn L, Bland B, Bochner B, Bogue L, Bork R, Bose S, Brady PR, Braginsky VB, Brau JE, Brown DA, Bullington A, Bunkowski A, Buonanno A, Burgess R, Busby D, Butler WE, Byer RL, Cadonati L, Cagnoli G, Camp JB, Cannizzo J, Cannon K, Cantley CA, Cao J, Cardenas L, Carter K, Casey MM, Castiglione J, Chandler A, Chapsky J, Charlton P, Chatterji S, Chelkowski S, Chen Y, Chickarmane V, Chin D, Christensen N, Churches D, Cokelaer T, Colacino C, Coldwell R, Coles M, Cook D, Corbitt T, Coyne D, Creighton JDE, Creighton TD, Crooks DRM, Csatorday P, Cusack BJ, Cutler C, Dalrymple J, D'Ambrosio E, Danzmann K, Davies G, Daw E, DeBra D, Delker T, Dergachev V, Desai S, DeSalvo R, Dhurandhar S, Di Credico A, Diaz M, Ding H, Drever RWP, Dupuis RJ, Edlund JA, Ehrens P, Elliffe EJ, Etzel T, Evans M, Evans T, Fairhurst S, Fallnich C, Farnham D, Fejer MM, Findley T, Fine M, Finn LS, Franzen KY, Freise A, Frey R, Fritschel P, Frolov VV, Fyffe M, Ganezer KS, Garofoli J, Giaime JA, Gillespie A, Goda K, Goggin L, Gonzalez G, Gossler S, Grandclement P, Grant A, Gray C, Gretarsson AM, Grimmett D, Grote H, Grunewald S, Guenther M, Gustafson E, Gustafson R, Hamilton WO, Hammond M, Hanna C, Hanson J, Hardham C, Harms J, Harry G, Hartunian A, Heefner J, Hefetz Y, Heinzel G, Heng IS, Hennessy M, Hepler N, Heptonstall A, Heurs M, Hewitson M, Hild S, Hindman N, Hoang P, Hough J, Hrynevych M, Hua W, Ito M, Itoh Y, Ivanov A, Jennrich O, Johnson B, Johnson WW, Johnston WR, Jones DI, Jones G, Jones L, Jungwirth D, Kalogera V, Katsavounidis E, Kawabe K, Kells W, Kern J, Khan A, Killbourn S, Killow CJ, Kim C, King C, King P, Klimenko S, Koranda S, Kotter K, Kovalik J, Kozak D, Krishnan B, Landry M, Langdale J, Lantz B, Lawrence R, Lazzarini A, Lei M, Leonor I, Libbrecht K, Libson A, Lindquist P, Liu S, Logan J, Lormand M, Lubinski M, Luck H, Luna M, Lyons TT, Machenschalk B, MacInnis M, Mageswaran M, Mailand K, Majid W, Malec M, Mandic V, Mann F, Marin A, Marka S, Maros E, Mason J, Mason K, Matherny O, Matone L, Mavalvala N, McCarthy R, McClelland DE, McHugh M, McNabb JWC, Melissinos A, Mendell G, Mercer RA, Meshkov S, Messaritaki E, Messenger C, Mikhailov E, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Miyakawa O, Mohanty S, Moreno G, Mossavi K, Mueller G, Mukherjee S, Murray P, Myers E, Myers J, Nagano S, Nash T, Nayak R, Newton G, Nocera F, Noel JS, Nutzman P, Olson T, O'Reilly B, Ottaway DJ, Ottewill A, Ouimette D, Overmier H, Owen BJ, Pan Y, Papa MA, Parameshwaraiah V, Parameswariah C, Pedraza M, Penn S, Pitkin M, Plissi M, Prix R, Quetschke V, Raab F, Radkins H, Rahkola R, Rakhmanov M, Rao SR, Rawlins K, Ray-Majumder S, Re V, Redding D, Regehr MW, Regimbau T, Reid S, Reilly KT, Reithmaier K, Reitze DH, Richman S, Riesen R, Riles K, Rivera B, Rizzi A, Robertson DI, Robertson NA, Robinson C, Robison L, Roddy S, Rodriguez A, Rollins J, Romano JD, Romie J, Rong H, Rose D, Rotthoff E, Rowan S, Rudiger A, Ruet L, Russell P, Ryan K, Salzman I, Sandberg V, Sanders GH, Sannibale V, Sarin P, Sathyaprakash B, Saulson PR, Savage R, Sazonov A, Schilling R, Schlaufman K, Schmidt V, Schnabel R, Schofield R, Schutz BF, Schwinberg P, Scott SM, Seader SE, Searle AC, Sears B, Seel S, Seifert F, Sellers D, Sengupta AS, Shapiro CA, Shawhan P, Shoemaker DH, Shu QZ, Sibley A, Siemens X, Sievers L, Sigg D, Sintes AM, Smith JR, Smith M, Smith MR, Sneddon PH, Spero R, Spjeld O, Stapfer G, Steussy D, Strain KA, Strom D, Stuver A, Summerscales T, Sumner MC, Sung M, Sutton PJ, Sylvestre J, Tanner DB, Tariq H, Tarallo M, Taylor I, Taylor R, Taylor R, Thorne KA, Thorne KS, Tibbits M, Tilav S, Tinto M, Tokmakov KV, Torres C, Torrie C, Traylor G, Tyler W, Ugolini D, Ungarelli C, Vallisneri M, van Putten M, Vass S, Vecchio A, Veitch J, Vorvick C, Vyachanin SP, Wallace L, Walther H, Ward H, Ward R, Ware B, Watts K, Webber D, Weidner A, Weiland U, Weinstein A, Weiss R, Welling H, Wen L, Wen S, Wette K, Whelan JT, Whitcomb SE, Whiting BF, Wiley S, Wilkinson C, Willems PA, Williams PR, Williams R, Willke B, Wilson A, Winjum BJ, Winkler W, Wise S, Wiseman AG, Woan G, Woods D, Wooley R, Worden J, Wu W, Yakushin I, Yamamoto H, Yoshida S, Zaleski KD, Zanolin M, Zawischa I, Zhang L, Zhu R, Zotov N, Zucker M, Zweizig J, Akutsu T, Akutsu T, Ando M, Arai K, Araya A, Asada H, Aso Y, Beyersdorf P, Fujiki Y, Fujimoto MK, Fujita R, Fukushima M, Futamase T, Hamuro Y, Haruyama T, Hayama K, Iguchi H, Iida Y, Ioka K, Ishizuka H, Kamikubota N, Kanda N, Kaneyama T, Karasawa Y, Kasahara K, Kasai T, Katsuki M, Kawamura S, Kawamura M, Kawazoe F, Kojima Y, Kokeyama K, Kondo K, Kozai Y, Kudoh H, Kuroda K, Kuwabara T, Matsuda N, Mio N, Miura K, Miyama S, Miyoki S, Mizusawa H, Moriwaki S, Musha M, Nagayama Y, Nakagawa K, Nakamura T, Nakano H, Nakao K, Nishi Y, Numata K, Ogawa Y, Ohashi M, Ohishi N, Okutomi A, Oohara K, Otsuka S, Saito Y, Sakata S, Sasaki M, Sato N, Sato S, Sato Y, Sato K, Sekido A, Seto N, Shibata M, Shinkai H, Shintomi T, Soida K, Somiya K, Suzuki T, Tagoshi H, Takahashi H, Takahashi R, Takamori A, Takemoto S, Takeno K, Tanaka T, Taniguchi K, Tanji T, Tatsumi D, Telada S, Tokunari M, Tomaru T, Tsubono K, Tsuda N, Tsunesada Y, Uchiyama T, Ueda K, Ueda A, Waseda K, Yamamoto A, Yamamoto K, Yamazaki T, Yanagi Y, Yokoyama J, Yoshida T, Zhu ZH

    PHYSICAL REVIEW D   72 ( 12 )   2005.12( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.72.122004

  • Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts Reviewed

    Abbott B, Abbott R, Adhikari R, Ageev A, Agresti J, Ajith P, Allen B, Allen J, Amin R, Anderson SB, Anderson WG, Araya M, Armandula H, Ashley M, Asiri F, Aufmuth P, Aulbert C, Babak S, Balasubramanian R, Ballmer S, Barish BC, Barker C, Barker D, Barnes M, Barr B, Barton MA, Bayer K, Beausoleil R, Belczynski K, Bennett R, Berukoff SJ, Betzwieser J, Bhawal B, Bilenko IA, Billingsley G, Black E, Blackburn K, Blackburn L, Bland B, Bochner B, Bogue L, Bork R, Bose S, Brady PR, Braginsky VB, Brau JE, Kanda N

    PHYSICAL REVIEW D   72 ( 12 )   2005.12( ISSN:2470-0010 ( eISSN:1550-2368

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    DOI: 10.1103/PhysRevD.72.122004

    Other URL: http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.72.122004/fulltext

  • Black-hole ringdown search in TAMA300: matched filtering and event selections Reviewed

    Tsunesada Y, Kanda N, Nakano H, Tatsumi D

    CLASSICAL AND QUANTUM GRAVITY   22 ( 18 )   S1129 - S1138   2005.09( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/22/18/S27

  • Upper limits on gravitational-wave bursts radiated from stellar-core collapses in our galaxy Reviewed

    Ando M, Akutsu T, Akutsu T, Arai K, Aso Y, Fukushima M, Hayama K, Kanda N, Kondo K, Mio N, Miyoki S, Moriwaki S, Nagano S, Sato S, Shibata M, Tagoshi H, Takahashi H, Takahashi R, Tatsumit D, Tsunesada Y, Yamazaki T

    CLASSICAL AND QUANTUM GRAVITY   22 ( 18 )   S1283 - S1291   2005.09( ISSN:0264-9381

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    DOI: 10.1088/0264-93891/22/18/S42

  • Calibration of TAMA300 in time domain Reviewed

    Telada S, Tatsumi D, Akutsu T, Ando M, Kanda N

    CLASSICAL AND QUANTUM GRAVITY   22 ( 18 )   S975 - S984   2005.09( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/22/18/S11

  • Burst wave analysis of TAMA300 data with the ALF filter Reviewed

    Akutsu T, Ando M, Kanda N, Tatsumi D, Telada S, Hayakawa H, Yamamoto K, Miyoki S, Ohashi M, Kuroda K

    CLASSICAL AND QUANTUM GRAVITY   22 ( 18 )   S1303 - S1309   2005.09( ISSN:0264-9381

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    DOI: 10.1088/0264-9381/22/18/S44

  • Calibration of TAMA300 in time domain Reviewed

    Souichi Telada, Daisuke Tatsumi, Tomomi Akutsu, Masaki Ando, Nobuyuki Kanda

    Classical and Quantum Gravity   22 ( 18 )   S975 - S984   2005.09( ISSN:0264-9381

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    We could reconstruct the strain of gravitational wave signals from acquired data in the time domain by using the infinite impulse response filter technique in TAMA300. We would like to analyse the waveform in the time domain for burst-like signal, merger phase waveform of binary neutron stars, and so on. We established the way to make a continuous time-series gravitational wave strain signal. We compared the time-domain reconstruction with the Fourier-space reconstruction. Both coincided within 3% in the observation range. We could also produce the voltage signal which would be recorded by the data-acquisition system from a simulated gravitational wave. This is useful for some analyses of simulations and signal injections. We could extract the waveform of the hardware injection signal in an observational run in the time domain. The extracted waveform was similar to the injection signal. © 2005 IOP Publishing Ltd.

    DOI: 10.1088/0264-9381/22/18/S11

  • Black-hole ringdown search in TAMA300: matched filtering and event selections Reviewed

    Yoshiki Tsunesada, Nobuyuki Kanda, Hiroyuki Nakano, Daisuke Tatsumi, The TAMA collaboration

    Class. Quantum Grav.   22   S1129   2005.09

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    DOI: 10.1088/0264-9381/22/18/S27

  • On detection of black hole quasinormal ringdowns: Detection efficiency and waveform parameter determination in matched filtering Reviewed

    Tsunesada Y, Kanda N, Nakano H, Tatsumi D, Ando M, Sasaki M, Tagoshi H, Takahashi H

    PHYSICAL REVIEW D   71 ( 10 )   2005.05( ISSN:1550-7998

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.1103/PhysRevD.71.103005

  • On detection of black hole quasinormal ringdowns: Detection efficiency and waveform parameter determination in matched filtering Reviewed

    Yoshiki Tsunesada, Nobuyuki Kanda, Hiroyuki Nakano, Daisuke Tatsumi, Masaki Ando, Misao Sasaki, Hideyuki Tagoshi, Hirotaka Takahashi

    Phys. Rev. D   71   103005 - 103005   2005.05

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    DOI: 10.1103/PhysRevD.71.103005

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  • Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses Reviewed

    Ando M, Arai K, Aso Y, Beyersdorf P, Hayama K, Iida Y, Kanda N, Kawamura S, Kondo K, Mio N, Miyoki S, Moriwaki S, Nagano S, Numata K, Sato S, Somiya K, Tagoshi H, Takahashi H, Takahashi R, Tatsumi D, Tsunesada Y, Zhu ZH, Akutsu T, Akutsu T, Araya A, Asada H, Barton MA, Fujiki Y, Fujimoto MK, Fujita R, Fukushima M, Futamase T, Hamuro Y, Haruyama T, Hayakawa H, Heinzel G, Horikoshi G, Iguchi H, Ioka K, Ishitsuka H, Kamikubota N, Kaneyama T, Karasawa Y, Kasahara K, Kasai T, Katsuki M, Kawabe K, Kawamura M, Kawashima N, Kawazoe F, Kojima Y, Kokeyama K, Kozai Y, Kudoh H, Kuroda K, Kuwabara T, Matsuda N, Miura K, Miyakawa O, Miyama S, Mizusawa H, Musha M, Nagayama Y, Nakagawa K, Nakamura T, Nakano H, Nakao K, Nishi Y, Ogawa Y, Ohashi M, Ohishi N, Okutomi A, Oohara K, Otsuka S, Saito Y, Sakata S, Sasaki M, Sato K, Sato N, Sato Y, Seki H, Sekido A, Seto N, Shibata M, Shinkai H, Shintomi T, Soida K, Suzuki T, Takamori A, Takemoto S, Takeno K, Tanaka T, Taniguchi K, Taniguchi S, Tanji T, Taylor CT, Telada S, Tochikubo K, Tokunari M, Tomaru T, Tsubono K, Tsuda N, Uchiyama T, Ueda A, Ueda K, Usui F, Waseda K, Watanabe Y, Yakura H, Yamamoto A, Yamamoto K, Yamazaki T, Yanagi Y, Yoda T, Yokoyama J, Yoshida T

    PHYSICAL REVIEW D   71 ( 8 )   2005.04( ISSN:2470-0010

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    DOI: 10.1103/PhysRevD.71.082002

  • Black hole ringdown search in TAMA300: Matched filtering and event selections

    Class. Quant. Grav.   22 ( 18 )   S1129   2005

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  • Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses, Reviewed

    Phys. Rev. D   71   82002   2005

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  • On Detection of Black Hole Quasi-Normal Ringdowns: Detection Efficiency and Waveform Parameter Determination in Matched Filtering,

    Phys.Rev. D   71   103005   2005

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  • Upper limits on gravitational-wave bursts radiated from stellar-core collapses in our galaxy Reviewed

    Ando M, Akutsu T, Arai K, Aso Y, Fukushima M, Hayama K, Kanda N, Kondo K, Mio N, Miyoki S, Moriwaki S, Nagano S, Sato S, Shibata M, Tagoshi H, Takahashi H, Takahashi R, Tatsumit D, Tsunesada Y, Yamazaki T, TAMA Collaboration

    Classical and Quantum Gravity   22 ( 18 )   S1283 - S1291   2005

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    DOI: 10.1088/0264-9381/22/18/S42

    Other URL: http://orcid.org/0000-0002-8865-9998

  • 26pXH-9 Power recycling of TAMA300, a 300m laser interferometer gravitational wave detector XVIII (Modulation-demodulation related noise) Reviewed

    Sato S., Miyoki S., Nagano S., Ando M., Moriwaki S., Musha M., Kanda N., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Arai K., Ohashi M., Kuroda K., the TAMA Collaboration, Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.1.1.0_98_1

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  • 26pXH-8 Power recycling of TAMA300, a 300-m laser interferometer gravitational wave XVII (detector improvement) Reviewed

    Arai K., Miyoki S., Nagano S., Ando M., Moriwaki S., Musha M., Kanda N., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Sato S., Ohashi M., Kuroda K., TAMA Collaboration, Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fnkushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.1.1.0_97_4

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  • 26pXH-3 Burst gravitational wave search with TAMA300, a 300-m laser interferometric gravitational wave detector IV Reviewed

    Ando M., Mio N., Moriwaki S., Miyoki S., Kondo K., Aso Y., Akutsu T., Nagano S., TAMA collaboration, Takahashi R., Arai K., Sato S., Tatsumi D., Kanda N., Tsunesada Y., Yamazaki T., Fukushima M.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.1.1.0_97_1

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  • 26pXH-2 Current states of Burst analysis of TAMA 300 data with the ALF filter Reviewed

    Akutsu T., Kuroda K., Ando M., Kanda N., Tatsumi D., Telada S., Hayakawa H., Yamamoto K., Miyoki S., Ohashi M.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.1.1.0_96_3

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  • 26pXH-10 Power recycling of TAMA300, a 300-m laser interferometric gravitational wave detector XIV (Signal, Control) Reviewed

    Nakagawa N., Miyoki S., Nagano S., Ando M., Moriwaki S., Musha M., Kanda N., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Arai K., Ohashi M., Kuroda K., TAMA Collaboration, Sato S., Takahashi R., Akustu T., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.1.1.0_98_2

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  • 15aSF-7 Development status of the interferometric gravitational wave detector TAMA300 III : Modulation-demodulation related noise Reviewed

    Sato S., Takamori A., Iida H., Bertolini A., DeSalvo R., Miyoki S., Nagano S., Ando M., Moriwaki N., Kanda N., Musha M., Arai K., Mio N., Kawamura S., Fujimoto M.K., Tsubono K., Ohashi M., Kuroda K., TAMA Collaboration, Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.2.1.0_38_3

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  • 15aSF-6 Status of Development for Interferometric Gravitational Wave Detector TAMA300 II : Interferometer Development Reviewed

    Arai K., Takamori A., Iida H., Bertolini A., DeSalvo R., Miyoki S., Nagano S., Ando M., Moriwaki N., Kanda N., Musha M., Sato S., Mio N., Kawamura S., Fujimoto M.K., Tsubono K., Ohashi M., Kuroda K., TAMA Collaboration, Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.2.1.0_38_2

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  • 15aSF-4 Burst gravitational wave search with TAMA300, a 300-m laser interferometric gravitational wave detector V Reviewed

    Ando M., Mio N., Miyoki S., Moriwaki S., Nagano S., Sato S., Shibata M., Tagashi H., Takahashi H., Takahashi R., Tatsumi D., Akutsu T., Tsunesada Y., Yamazaki T., and the TAMA collaboration, Akutsu T., Arai K., Aso Y., Fukushima M., Hayama K., Kanda N., Kondo K.

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.2.1.0_37_4

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  • Upper limits on gravitational-wave bursts radiated from stellar-core collapses in our galaxy Reviewed

    Ando M, Akutsu T, Arai K, Aso Y, Fukushima M, Hayama K, Kanda N, Kondo K, Mio N, Miyoki S, Moriwaki S, Nagano S, Sato S, Shibata M, Tagoshi H, Takahashi H, Takahashi R, Tatsumit D, Tsunesada Y, Yamazaki T, TAMA Collaboration

    Classical and Quantum Gravity   22 ( 18 )   S1283 - S1291   2005( ISSN:0264-9381 ( eISSN:1361-6382

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    DOI: 10.1088/0264-9381/22/18/S42

    Other URL: http://orcid.org/0000-0002-8865-9998

  • Burst wave analysis of TAMA300 data with the ALF filter. Reviewed

    T.Akutsu, M.Ando, N.Kanda, D.Tatsumi, S.Telada, H.Hayakawa, K.Yamamoto, S.Miyoki, M.Ohashi, K.Kuroda, the TAMA Collaboration

    Classical and Quantum Gravity   22   S1303 - S1309   2005

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    DOI: 10.1088/0264-9381/22/18/S44

  • 26pXH-9 Power recycling of TAMA300, a 300m laser interferometer gravitational wave detector XVIII (Modulation-demodulation related noise)

    Sato S., Arai K., Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T., Miyoki S., Nagano S., Ando M., Moriwaki S., Musha M., Kanda N., Mio N., Kawamura S., Fujimoto M.-K., Tsubono K., Ohashi M., Kuroda K., the TAMA Collaboration

    Meeting Abstracts of the Physical Society of Japan   60.1.1 ( 0 )   98   2005( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.1.1.0_98_1

    CiNii Article

  • 26pXH-8 レーザー干渉計型重力波検出器TAMA300のパワーリサイクリングXVII(検出器改良)(重力波,宇宙線・宇宙物理) Reviewed

    新井 宏二, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 佐藤 修一, 大橋 正健, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   60 ( 0 )   97 - 97   2005( ISSN:1342-8349 ( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.1.1.0_97_4

    CiNii Article

  • 26pXH-3 TAMA300データを用いたバースト重力波解析IV(重力波,宇宙線・宇宙物理) Reviewed

    安東 花樹, 三尾 典克, 森脇 成典, 三代木 伸二, 近藤 寿浩, 麻生 洋一, 阿久津 智忠, 長野 重夫, TAMA Collaboration, 高橋 竜太郎, 新井 宏二, 佐藤 修一, 辰巳 大輔, 神田 展行, 常定 芳基, 山崎 利孝, 福嶋 美津広

    一般社団法人 日本物理学会 日本物理学会講演概要集   60 ( 0 )   97 - 97   2005( ISSN:1342-8349 ( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.1.1.0_97_1

    CiNii Article

  • 26pXH-2 Current states of Burst analysis of TAMA 300 data with the ALF filter

    Akutsu T., Ando M., Kanda N., Tatsumi D., Telada S., Hayakawa H., Yamamoto K., Miyoki S., Ohashi M., Kuroda K.

    Meeting Abstracts of the Physical Society of Japan   60.1.1 ( 0 )   96   2005( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.1.1.0_96_3

    CiNii Article

  • 26pXH-10 レー-ザー干渉計型重力波検出器TAMA300のパワーリサイクリングXIX(信号取得・制御系)(重力波,宇宙線・宇宙物理) Reviewed

    中川 憲保, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 新井 宏二, 大橋 正健, 黒田 和明, TAMA Collaboration, 佐藤 修一, 高橋 竜太郎, 阿久津 智忠, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   60 ( 0 )   98 - 98   2005( ISSN:1342-8349 ( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.1.1.0_98_2

    CiNii Article

  • 15aSF-7 Development status of the interferometric gravitational wave detector TAMA300 III : Modulation-demodulation related noise

    Sato S., Arai K., Takahashi R., Akutsu T., Nakagawa N., Tatsumi D., Tsunesada Y., Fukushima M., Yamazaki T., Takamori A., Iida H., Bertolini A., DeSalvo R., Miyoki S., Nagano S., Ando M., Moriwaki N., Kanda N., Musha M., Mio N., Kawamura S., Fujimoto M.K., Tsubono K., Ohashi M., Kuroda K., TAMA Collaboration

    Meeting Abstracts of the Physical Society of Japan   60.2.1 ( 0 )   38   2005( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.2.1.0_38_3

    CiNii Article

  • 15aSF-6 干渉計型重力波検出器TAMA300開発の現状II : 干渉計開発(15aSF 重力波,宇宙線・宇宙物理領域) Reviewed

    新井 宏二, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 佐藤 修一, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正雄, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   60 ( 0 )   38 - 38   2005( ISSN:1342-8349 ( eISSN:21890803

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    Publishing type:Research paper (scientific journal)  

    DOI: 10.11316/jpsgaiyo.60.2.1.0_38_2

    CiNii Article

  • Plans for the LIGO-TAMA Joint Search for Gravitational Wave Bursts,

    Class. Quant. Grav.   21   S1801   2004

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  • Coincidence analysis to search for inspiraling compact binaries using TAMA300 and LISM data,

    Phys. Rev. D   70   42003   2004

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    Publishing type:Research paper (scientific journal)  

  • First search for gravitational waves from inspiraling compact binaries using TAMA300 data

    Phys. Rev. D   63   62001   2001

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  • Stable Operation of a 300-m Laser Interferometer with Sufficient Sensitivity to Detect Gravitational Wave Events within Our Galaxy

    Physical Review Letters   86   3950 - 3954   2001

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▼display all

Books and Other Publications

  • 宇宙物理学ハンドブック

    高原文郎, 家正則, 小玉英雄, 高橋忠幸 編( Role: Joint author)

    朝倉書店  2020.02 

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    Total pages:896   Responsible for pages:8  

  • 宇宙物理学ハンドブック

    高原文郎, 家正則, 小玉英雄, 高橋忠幸( Role: Sole author)

    朝倉書店  2020.02 

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    Total pages:896   Responsible for pages:8   Book type:Scholarly book

  • 宇宙物理学ハンドブック

    高原文郎, 家正則, 小玉英雄, 高橋忠幸( Role: Joint author)

    朝倉書店  2020.02 

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    Total pages:896   Responsible for pages:8   Book type:Scholarly book

MISC

  • Building a Low Latency Data Sharing System in the International Gravitational Wave Observation Network with Apache Kafka Reviewed

    小根澤瞭太, BROCKILL Patrick J, 神田展行, 大原謙一, 土田怜, 酒井一樹

    日本物理学会講演概要集(CD-ROM)   76 ( 1 )   2021( ISSN:2189-079X

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)  

    J-GLOBAL

  • Hilbert-Huang変換を用いた重力波カタログイベントの解析 Reviewed

    武田芽依, 神田展行, 大原謙一, 高橋弘毅, 酒井一樹, 日下公亨, 豊島弥洋

    日本物理学会講演概要集(CD-ROM)   76 ( 1 )   2021( ISSN:2189-079X

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    J-GLOBAL

  • Hilbert-Huang変換を用いた重力崩壊型超新星爆発由来の重力波データ解析 Reviewed

    武田芽依, 渡邊幸伸, 平沼悠太, 根岸諒, 大原謙一, 神田展行, 黒田仰生, 固武慶, 酒井一樹, 坂井佑輔, 澤田崇広, 高橋弘毅, 滝脇知也, 土田怜, 端山和大, 横澤孝章

    日本天文学会年会講演予稿集   2021   2021( ISSN:1347-0639

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    J-GLOBAL

  • Hilbert-Huang変換を用いた重力波カタログイベントの解析 Reviewed

    武田芽依, 神田展行, 大原謙一, 高橋弘毅, 酒井一樹, 日下公亨, 豊島弥洋

    日本物理学会講演概要集(CD-ROM)   76 ( 1 )   2021( ISSN:2189-079X

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    J-GLOBAL

  • Hilbert-Huang変換を用いた重力崩壊型超新星爆発由来の重力波データ解析 Reviewed

    武田芽依, 渡邊幸伸, 平沼悠太, 根岸諒, 大原謙一, 神田展行, 黒田仰生, 固武慶, 酒井一樹, 坂井佑輔, 澤田崇広, 高橋弘毅, 滝脇知也, 土田怜, 端山和大, 横澤孝章

    日本天文学会年会講演予稿集   2021   2021( ISSN:1347-0639

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)  

    J-GLOBAL

  • Building a Low Latency Data Sharing System in the International Gravitational Wave Observation Network with Apache Kafka Reviewed

    小根澤瞭太, BROCKILL Patrick J, 神田展行, 大原謙一, 土田怜, 酒井一樹

    日本物理学会講演概要集(CD-ROM)   76 ( 1 )   2021( ISSN:2189-079X

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)  

    J-GLOBAL

  • Hilbert-Huang変換を用いた,重力崩壊型超新星爆発のSASI由来の重力波解析 Reviewed

    武田芽依, 渡邊幸伸, 平沼悠太, 根岸諒, 大原謙一, 神田展行, 黒田仰生, 固武慶, 酒井一樹, 坂井佑輔, 澤田崇広, 高橋弘毅, 滝脇知也, 土田怜, 端山和大, 横澤孝章

    日本物理学会講演概要集(CD-ROM)   75 ( 1 )   2020( ISSN:2189-079X

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    J-GLOBAL

  • Hilbert-Huang変換を用いた,重力崩壊型超新星爆発のSASI由来の重力波解析 Reviewed

    武田芽依, 渡邊幸伸, 平沼悠太, 根岸諒, 大原謙一, 神田展行, 黒田仰生, 固武慶, 酒井一樹, 坂井佑輔, 澤田崇広, 高橋弘毅, 滝脇知也, 土田怜, 端山和大, 横澤孝章

    日本物理学会講演概要集(CD-ROM)   75 ( 1 )   2020( ISSN:2189-079X

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    J-GLOBAL

  • 重力波観測が明らかにする中性子星連星の姿 Invited

    神田展行

    天文月報   111 ( 1 )   8 - 10   2018

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)   Kind of work:Single Work  

  • 重力波観測が明らかにする中性子星連星の姿 Reviewed

    神田展行

    天文月報   111 ( 1 )   8 - 10   2018

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  • 重力波観測が明らかにする中性子星連星の姿 Invited

    神田展行

    天文月報   111 ( 1 )   8 - 10   2018

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  • Expectation for the coincidence / follow-up observations by electromagnetic waves for gravitational wave events Invited

    Nobuyuki Kanda

    110 ( 1 )   6 - 13   2017

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  • Expectation for the coincidence / follow-up observations by electromagnetic waves for gravitational wave events Reviewed

    Nobuyuki Kanda

    110 ( 1 )   6 - 13   2017

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  • Expectation for the coincidence / follow-up observations by electromagnetic waves for gravitational wave events Invited

    Nobuyuki Kanda

    110 ( 1 )   6 - 13   2017( ISSN:0374-2466

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    CiNii Article

  • 初観測された重力波が開いた宇宙への新しい窓 Invited

    神田展行

    雑誌パリティ(丸善出版)   ( 10 )   2016

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)   Kind of work:Single Work  

  • 重力波の発見:一般相対性理論の100年後の証明 Invited

    神田展行

    雑誌パリティ(丸善出版)   ( 6 )   2016

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)   Kind of work:Single Work  

  • 初観測された重力波が開いた宇宙への新しい窓 Reviewed

    神田展行

    雑誌パリティ(丸善出版)   ( 10 )   2016

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)   Kind of work:Single Work  

  • 重力波の発見:一般相対性理論の100年後の証明 Reviewed

    神田展行

    雑誌パリティ(丸善出版)   ( 6 )   2016

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)   Kind of work:Single Work  

  • 初観測された重力波が開いた宇宙への新しい窓 Invited

    神田展行

    雑誌パリティ(丸善出版)   31 ( 10 )   14 - 18   2016( ISSN:0911-4815

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    CiNii Article

  • 重力波の発見:一般相対性理論の100年後の証明 Invited

    神田展行

    雑誌パリティ(丸善出版)   31 ( 6 )   40 - 42   2016( ISSN:0911-4815

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    CiNii Article

  • 22pDJ-13 神岡におけるシューマン共振の測定 Reviewed

    熱田 将, 齊藤 芳男, 宗宮 健太郎, 西澤 篤志, 宮川 治, 三代木 伸二, 矢野 和城, 小河 勉, 山口 覚, 端山 和大, 新谷 昌人, 上嶋 誠, 内山 隆, 小野 謙次, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集   70   2015

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    DOI: 10.11316/jpsgaiyo.70.1.0_449

  • 22pDJ-13 神岡におけるシューマン共振の測定 Reviewed

    熱田 将, 齊藤 芳男, 宗宮 健太郎, 西澤 篤志, 宮川 治, 三代木 伸二, 矢野 和城, 小河 勉, 山口 覚, 端山 和大, 新谷 昌人, 上嶋 誠, 内山 隆, 小野 謙次, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集   70 ( 0 )   449 - 449   2015( ISSN:2189-079X ( eISSN:21890803

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    Publishing type:Article, review, commentary, editorial, etc. (scientific journal)  

    DOI: 10.11316/jpsgaiyo.70.1.0_449

    CiNii Article

  • 20aSB-1 大型低温重力波望遠鏡(KAGRA)プロジェクトの現状(20aSB 重力波(KAGRA),宇宙線・宇宙物理領域) Reviewed

    麻生 洋一, 梶田 隆章, 黒田 和明, 大橋 正健, 川村 静児, 三代木 伸二, 内山 隆, 宮川 治, 齋藤 芳男, 大石 奈緒子, 山元 一広, Khalaidovski Alexandar, Kumar Rahul, 大嶋 新一, 石塚 秀喜, 廣瀬 榮一, 上泉 眞裕, 榊原 裕介, 関口 貴令, 陳 タン, 中野 雅之, 小野 謙次, 小仁所 志栞, 西村 翼, 渡辺 篤, 山中 祐治, 宮本 昴拓, 田中 宏樹, 藤本 眞克, Flaminio Raffaele, 高橋 竜太郎, 上田 暁俊, 阿久津 智忠, 辰巳 大輔, 中村 康二, Arellano Fabian Pena, 石崎 秀晴, 鳥居 泰男, 田中 伸幸, 山本 明, 鈴木 敏一, 木村 誠宏, 都丸 隆行, 井岡 邦仁, 久米 達哉, 小池 重明, 横山 順一, 伊藤 洋介, 枝 和成, 坪野 公夫, 安東 正樹, 平松 成範, 穀山 渉, 岡田 健志, 松本 伸之, 道村 唯太, 正田 亜八香, 柴田 和憲, 牛場 崇文, 渡部 恭平, 三尾 典克, 大前 宣昭, 鈴木 健一郎, 古谷 寛之, 細谷 暁夫, 河合 誠之, 宗宮 健太郎, 須佐 友紀, 上田 慎一郎, 加藤 準平, 粂田 綾香, 神田 展行, 端山 和大, 横澤 孝章, 山本 尚弘, 譲原 浩貴, 田中 一幸, 浅野 光洋, 鳥谷 仁人, 有馬 司, 宮本 晃伸, 中尾 憲一, 中村 卓史, 田中 貴浩, 瀬戸 直樹, 西澤 篤志, 植田 憲一, 米田 仁紀, 中川 賢一, 武者 満, 新谷 昌人, 高森 昭光, 佐藤 修一, 林 翔平, 奥富 弘基, 高辻 利之, 尾藤 洋一, 寺田 聡一, 長野 重夫, 田越 秀行, 上野 昂, 成川 達也, 佐野 保道, 高倉 理, Baiotti Luca, 佐々木 節, 柴田 大, 樽家 篤史, 中野 寛之, 関口 雄一郎, 佐合 紀親, 斎藤 那菜, 新冨 孝和, 大原 謙一, 金山 雅人, 若松 剛司, 佐藤 孝, 大河 正志, 土井 康平, 齊藤 高大, 飯島 音浩, 志賀 和成, 高橋 弘毅, 姫本 宣朗, 浅田 秀樹, 二間瀬 敏史, 高橋 史宜, 原田 知広, 小嶌 康史, 瓜生 康史, 山田 章一, 西條 統之, 大森 隆夫, 松島 房和, 森脇 喜紀, 小林 かおり, 榎本 勝成, 大石 諒, 〓ノ下 陽哉, 柿崎 充, 小野 行徳, 堀 匡寛, 早川 陽介, 廣林 茂樹, 沖野 浩二, Ruggero Micheletto, 固武 慶, 江口 智士, 中谷 一郎, 阪田 紫帆里, 鹿野 豊, 春山 富義, 上原 知幸, 川添 史子, Chen Yanbei, 河邉 径太, 新井 宏二, Miao Haixing, 和泉 究, Tobar M.E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, 苔山 圭以子, Zhu Zong-Hong, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, 沼田 健司, Marka Szabolcs, Marka Zsuzsanna, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Matta Vincenzo, Postiglione Fabio, Longo Maurizio, Addesso Paolo, Fusco Adele, Majorana Ettore, Zhai Xiang-hua, Xi Ping, Ni Wei-Tou, Mei Hsien-Hao, Yoon Tai Hyun, Lee Hyung Won, Kim Kyoung Yee, Kim Jeongcho, Lee Hyung Mok, Kim Chunglee, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, van Putten, Maurice H.P.M, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya, 樫山 和己, 八木 絢外, Pai Archana, 我妻 一博, 久徳 浩太郎

    一般社団法人日本物理学会 日本物理学会講演概要集   69 ( 2 )   2014.08( ISSN:1342-8349

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  • 21aSB-4 スペース重力波アンテナDECIGO計画(55) : DECIGO/DPFの概要(21aSB 重力波(KAGRA,DECIGO,TOBA,検出器),宇宙線・宇宙物理領域) Reviewed

    安東 正樹, 川村 静児, 瀬戸 直樹, 中村 卓史, 坪野 公夫, 佐藤 修一, 田中 貴浩, 船木 一幸, 沼田 健司, 神田 展行, 井岡 邦仁, 高島 健, 横山 順一, 阿久津 智忠, 武者 満, 上田 暁俊, 麻生 洋一, 新谷 昌人, 坂井 真一郎, 青柳 巧介, 我妻 一博, 浅田 秀樹, 新井 宏二, 池上 健, 石川 毅彦, 石崎 秀晴, 石原 秀樹, 和泉 究, 市來 淨與, 伊東 宏之, 伊藤 洋介, 井上 開輝, 植田 憲一, 牛場 崇文, 歌島 昌由, 江口 智士, 江尻 悠美子, 榎 基宏, 戎崎 俊一, 江里口 良治, 大石 奈緒子, 大河 正志, 大橋 正健, 大原 謙一, 大渕 喜之, 岡田 健志, 岡田 則夫, 奥富 弘基, 河島 信樹, 川添 史子, 河野 功, 木内 建太, 岸本 直子, 國中 均, 國森 裕生, 黒田 和明, 黒柳 幸子, 小泉 宏之, 洪 鋒雷, 郡 和範, 穀山 渉, 苔山 圭以子, 古在 由秀, 小嶌 康史, 固武 慶, 小林 史歩, 権藤 里奈, 西條 統之, 齊藤 遼, 阪上 雅昭, 阪田 紫帆里, 佐合 紀親, 佐々木 節, 佐藤 孝, 柴田 大, 柴田 和憲, 正田 亜八香, 真貝 寿明, 末正 有, 杉山 直, 鈴木 理恵子, 諏訪 雄大, 宗宮 健太郎, 祖谷 元, 高野 忠, 高橋 走, 高橋 慶太郎, 高橋 弘毅, 高橋 史宜, 高橋 龍一, 高橋 竜太郎, 高森 昭光, 田越 秀行, 田代 寛之, 田中 伸幸, 谷口 敬介, 樽家 篤史, 千葉 剛, 陳 たん, 辻川 信二, 常定 芳基, 豊嶋 守生, 鳥居 泰男, 中尾 憲一, 中澤 知洋, 中須賀 真一, 中野 寛之, 長野 重夫, 中村 康二, 中山 宜典, 西澤 篤志, 西田 恵里奈, 西山 和孝, 丹羽 佳人, 能見 大河, 橋本 樹明, 端山 和大, 原田 知広, 疋田 渉, 姫本 宣朗, 平林 久, 平松 尚志, 福嶋 美津広, 藤田 龍一, 藤本 眞克, 二間瀬 敏史, 細川 瑞彦, 堀澤 秀之, 前田 恵一, 松原 英雄, 松本 伸之, 道村 唯太, 宮川 治, 宮本 雲平, 三代木 伸二, 向山 信治, 森澤 理之, 森本 睦子, 森脇 成典, 八木 絢外, 山川 宏, 山崎 利孝, 山元 一広, 吉田 至順, 吉野 泰造, 柳 哲文, 若林 野花

    一般社団法人日本物理学会 日本物理学会講演概要集   69 ( 2 )   49 - 49   2014.08( ISSN:1342-8349

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  • 20pSB-8 Gravitational Wave Detection using Non-Harmonic Analysis(II) Reviewed

    Nakano Masaya, Hirobayashi Shigeki, Tagoshi Hideyuki, Kanda Nobuyuki, Hayama Kazuhiro, Kawamura Seiji, Miyake Kyohei

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   69 ( 2 )   47 - 47   2014.08( ISSN:1342-8349

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  • 20pSB-6 Investigation of Supernova explosion mechanism using detection simulation of Gravitational wave and Neutrino Reviewed

    Yokozawa T., Asano M., Arima T., Kayano T., Suwa Y., Kanda N., Koshio Y., Vagins M.

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   69 ( 2 )   47 - 47   2014.08( ISSN:1342-8349

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  • 20aSB-8 Control for KAGRA using digital system(VI) Reviewed

    Miyakawa O., Kamiizumi M., Sekiguchi T., Hayama K., Yokozawa T., Kanda N., Michimura Y., Miyoki S., Yamamoto T., Yuzurihara H., KAGRA Collaboration

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   69 ( 2 )   46 - 46   2014.08( ISSN:1342-8349

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  • 20aSB-8 Control for KAGRA using digital system(VI) Reviewed

    Miyakawa O., Kamiizumi M., Sekiguchi T., Hayama K., Yokozawa T., Kanda N., Michimura Y., Miyoki S., Yamamoto T., Yuzurihara H., KAGRA Collaboration

    Meeting abstracts of the Physical Society of Japan   69 ( 2 )   46 - 46   2014.08( ISSN:1342-8349

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  • 21aSB-4 スペース重力波アンテナDECIGO計画(55) : DECIGO/DPFの概要(21aSB 重力波(KAGRA,DECIGO,TOBA,検出器),宇宙線・宇宙物理領域) Reviewed

    安東 正樹, 川村 静児, 瀬戸 直樹, 中村 卓史, 坪野 公夫, 佐藤 修一, 田中 貴浩, 船木 一幸, 沼田 健司, 神田 展行, 井岡 邦仁, 高島 健, 横山 順一, 阿久津 智忠, 武者 満, 上田 暁俊, 麻生 洋一, 新谷 昌人, 坂井 真一郎, 青柳 巧介, 我妻 一博, 浅田 秀樹, 新井 宏二, 池上 健, 石川 毅彦, 石崎 秀晴, 石原 秀樹, 和泉 究, 市來 淨與, 伊東 宏之, 伊藤 洋介, 井上 開輝, 植田 憲一, 牛場 崇文, 歌島 昌由, 江口 智士, 江尻 悠美子, 榎 基宏, 戎崎 俊一, 江里口 良治, 大石 奈緒子, 大河 正志, 大橋 正健, 大原 謙一, 大渕 喜之, 岡田 健志, 岡田 則夫, 奥富 弘基, 河島 信樹, 川添 史子, 河野 功, 木内 建太, 岸本 直子, 國中 均, 國森 裕生, 黒田 和明, 黒柳 幸子, 小泉 宏之, 洪 鋒雷, 郡 和範, 穀山 渉, 苔山 圭以子, 古在 由秀, 小嶌 康史, 固武 慶, 小林 史歩, 権藤 里奈, 西條 統之, 齊藤 遼, 阪上 雅昭, 阪田 紫帆里, 佐合 紀親, 佐々木 節, 佐藤 孝, 柴田 大, 柴田 和憲, 正田 亜八香, 真貝 寿明, 末正 有, 杉山 直, 鈴木 理恵子, 諏訪 雄大, 宗宮 健太郎, 祖谷 元, 高野 忠, 高橋 走, 高橋 慶太郎, 高橋 弘毅, 高橋 史宜, 高橋 龍一, 高橋 竜太郎, 高森 昭光, 田越 秀行, 田代 寛之, 田中 伸幸, 谷口 敬介, 樽家 篤史, 千葉 剛, 陳 たん, 辻川 信二, 常定 芳基, 豊嶋 守生, 鳥居 泰男, 中尾 憲一, 中澤 知洋, 中須賀 真一, 中野 寛之, 長野 重夫, 中村 康二, 中山 宜典, 西澤 篤志, 西田 恵里奈, 西山 和孝, 丹羽 佳人, 能見 大河, 橋本 樹明, 端山 和大, 原田 知広, 疋田 渉, 姫本 宣朗, 平林 久, 平松 尚志, 福嶋 美津広, 藤田 龍一, 藤本 眞克, 二間瀬 敏史, 細川 瑞彦, 堀澤 秀之, 前田 恵一, 松原 英雄, 松本 伸之, 道村 唯太, 宮川 治, 宮本 雲平, 三代木 伸二, 向山 信治, 森澤 理之, 森本 睦子, 森脇 成典, 八木 絢外, 山川 宏, 山崎 利孝, 山元 一広, 吉田 至順, 吉野 泰造, 柳 哲文, 若林 野花

    日本物理学会講演概要集   69 ( 2 )   49 - 49   2014.08( ISSN:1342-8349

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  • 20pSB-8 Gravitational Wave Detection using Non-Harmonic Analysis(II) Reviewed

    Nakano Masaya, Hirobayashi Shigeki, Tagoshi Hideyuki, Kanda Nobuyuki, Hayama Kazuhiro, Kawamura Seiji, Miyake Kyohei

    Meeting abstracts of the Physical Society of Japan   69 ( 2 )   47 - 47   2014.08( ISSN:1342-8349

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  • 20pSB-6 Investigation of Supernova explosion mechanism using detection simulation of Gravitational wave and Neutrino Reviewed

    Yokozawa T., Asano M., Arima T., Kayano T., Suwa Y., Kanda N., Koshio Y., Vagins M.

    Meeting abstracts of the Physical Society of Japan   69 ( 2 )   47 - 47   2014.08( ISSN:1342-8349

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  • 27aTL-1 大型低温重力波望遠鏡(KAGRA)プロジェクトの現状(27aTL 重力波(KAGRA),宇宙線・宇宙物理領域) Reviewed

    安東 正樹, 梶田 隆章, 黒田 和明, 大橋 正健, 川村 静児, 三代木 伸二, 内山 隆, 宮川 治, 大石 奈緒子, 山元 一広, Khalaidovski Alexandar, Kumar Rahul, 西田 恵里奈, 石塚 秀喜, 東谷 千比呂, 廣瀬 榮一, 上泉 眞裕, 岩崎 詩子, 榊原 裕介, 関口 貴令, 陳 タン, 中野 雅之, 手嶋 航大, 小野 謙次, 小仁所 志栞, 西村 翼, 渡辺 篤, 藤本 眞克, Flaminio Raffaele, 高橋 竜太郎, 上田 暁俊, 阿久津 智忠, 辰巳 大輔, 中村 康二, Arellano Fabian Pena, Friedrich Daniel, 石崎 秀晴, 鳥居 泰男, 田中 伸幸, 奥冨 弘基, 江口 智士, 山本 明, 鈴木 敏一, 木村 誠宏, 都丸 隆行, 井岡 邦仁, 齊藤 芳男, 久米 達哉, 小池 重明, 横山 順一, 樽家 篤史, 伊藤 洋介, 坪野 公夫, 麻生 洋一, 平松 成範, 穀山 渉, 岡田 健志, 松本 伸之, 道村 唯太, 正田 亜八香, 柴田 和憲, 牛場 崇文, 渡辺 恭平, 三尾 典克, 森脇 成典, 大前 宣昭, 千葉 智弘, 福本 展大, 鈴木 健一郎, 古谷 寛之, 細谷 暁夫, 河合 誠之, 宗宮 健太郎, 須佐 友紀, 上田 慎一郎, 加藤 準平, 粂田 綾香, 神田 展行, 端山 和大, 横澤 孝章, 山本 尚弘, 譲原 浩貴, 田中 一幸, 浅野 光洋, 鳥谷 仁人, 中尾 憲一, 中村 卓史, 瀬戸 直樹, 西澤 篤志, 植田 憲一, 米田 仁紀, 中川 賢一, 武者 満, 新谷 昌人, 高森 昭光, 佐藤 修一, 林 翔平, 東浦 孝典, 高辻 利之, 尾藤 洋一, 寺田 総一, 長野 重夫, 田越 秀行, 上野 昂, 成川 達也, 佐野 保道, 高倉 理, Baiotti Luca, 佐々木 節, 柴田 大, 田中 貴浩, 中野 寛之, 関口 雄一郎, 佐合 紀親, 斎藤 那菜, 新冨 孝和, 大原 謙一, 平沼 悠太, 金山 雅人, 若松 剛司, 佐藤 孝, 大河 正志, 土井 康平, 前原 進也, 清水 直弥, 高橋 弘毅, 姫本 宣朗, 浅田 秀樹, 二間瀬 敏史, 高橋 史宜, 原田 知広, 小嶌 康史, 瓜生 康史, 山田 章一, 西條 統之, 大森 隆夫, 松島 房和, 森脇 喜紀, 小林 かおり, 榎本 勝成, 米山 直弥, 宮本 達也, 大石 諒, 〓ノ下 陽哉, 柿崎 充, 小野 行徳, 堀 匡寛, 早川 陽介, 廣林 茂樹, 沖野 浩二, Ruggero Micheletto, 固武 慶, 中谷 一郎, 阪田 紫帆里, 鹿野 豊, 春山 富義, 上原 知幸, 川添 史子, Chen Yanbei, 河邉 径太, 新井 宏二, Miao Haixing, 和泉 究, Tobar M.E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, 苔山 圭以子, Zhu Zong-Hong, Dhurandhar S, Mitra S, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, 沼田 健司, Marka Szabolcs, Marka Zsuzsanna, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Matta Vincenzo, Postiglione Fabio, Longo Maurizio, Addesso Paolo, Fusco Adele, Majorana Ettore, Zhai Xiang-hua, Xi Ping, Ni Wei-Tou, Mei Hsien-Hao, Wu Shan-Jyun, Yoon Tai Hyun, Lee Hyung Won, Kim Kyoung Yee, Kim Jeongcho, Lee Hyung Mok, Kim Chunglee, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, Putten Maurice, H.P.M. van, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya, 樫山 和己, 八木 絢外, Pai Archana, 我妻 一博, 久徳 浩太郎

    一般社団法人日本物理学会 日本物理学会講演概要集   69 ( 1 )   2014.03( ISSN:1342-8349

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  • 27pTL-10 Gravitational Wave Detection using Non-Harmonic Analysis Reviewed

    Nakano Masaya, Hirobayashi Shigeki, Tagoshi Hideyuki, Kanda Nobuyuki, Kawamura Seiji

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   69 ( 1 )   115 - 115   2014.03( ISSN:1342-8349

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  • 27pTL-10 Gravitational Wave Detection using Non-Harmonic Analysis Reviewed

    Nakano Masaya, Hirobayashi Shigeki, Tagoshi Hideyuki, Kanda Nobuyuki, Kawamura Seiji

    Meeting abstracts of the Physical Society of Japan   69 ( 1 )   115 - 115   2014.03( ISSN:1342-8349

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  • Control for KAGRA using digital system(V) Reviewed

    Miyakawa O, Aso Y, Izumi K, Ohishi N, Kamiizumi M, Kanda N, Tanaka K, Hayama K, Michimura Y, Miyoki S, Yamamoto T, Yuzurihara H, KAGRA Collaboration

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   68 ( 2 )   117 - 117   2013.08( ISSN:1342-8349

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  • Control for KAGRA using digital system(V) Reviewed

    Miyakawa O, Aso Y, Izumi K, Ohishi N, Kamiizumi M, Kanda N, Tanaka K, Hayama K, Michimura Y, Miyoki S, Yamamoto T, Yuzurihara H, KAGRA Collaboration

    Meeting abstracts of the Physical Society of Japan   68 ( 2 )   117 - 117   2013.08( ISSN:1342-8349

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  • 26aBE-1 The current status of Large-scale Cryogenic Gravitational Wave Telescope (KAGRA) Project (8) Reviewed

    Kawamura Seiji, Friedrich Daniel, Baiotti Luca, Chen Yanbei, Miao Haixing, Tobar M. E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, Zhu Zong-Hong, Dhurandhar S, Pai Archana, Mitra S, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, Marka Szabolcs, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Conte Roberto, Fiumara Vincenzo, Matta Vincenzo, Chiadini Francesco, Postiglione Fabio, Ni Wei-Tou, Zhai Xiang-hua, Xi Ping, Mei Hsien-Hao, Yoon Tai Hyun, Lee Hyung Won, Lee Hyung Mok, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, van Putten, Maurice H. P. M, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   68 ( 1 )   2013.03( ISSN:1342-8349

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  • 26pBE-3 Control for KAGRA using digital system (IV) Reviewed

    Miyakawa O., Aso Y., Izumi K., Uchiyama T., Ohishi N., Kamiizumi M., Kanda N., Tanaka K., Hayama K., Michimura Y., Miyoki S., Yamamoto T., Yuzurihara H., KAGRA Collaboration

    Meeting abstracts of the Physical Society of Japan   68 ( 1 )   122 - 122   2013.03( ISSN:1342-8349

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  • 26pBE-3 Control for KAGRA using digital system (IV) Reviewed

    Miyakawa O, Michimura Y, Miyoki S, Yamamoto T, Yuzurihara H, KAGRA Collaboration, Aso Y, Izumi K, Uchiyama T, Ohishi N, Kamiizumi M, Kanda N, Tanaka K, Hayama K

    The Physical Society of Japan, Meeting Abstracts of the Physical Society of Japan   68 ( 0 )   2013

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  • 11aSN-12 Control for KAGRA using digital system (III) Reviewed

    Miyakawa O., Aso Y., Izumi K., Ohishi N., Kamiizumi M., Kanda N., Hayama K., Michimura Y., Miyoki S., Yamamoto T., Yusurihara H.

    The Physical Society of Japan (JPS), Meeting abstracts of the Physical Society of Japan   67 ( 2 )   98 - 98   2012.08( ISSN:1342-8349

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  • 11aSN-12 Control for KAGRA using digital system (III) Reviewed

    Miyakawa O., Aso Y., Izumi K., Ohishi N., Kamiizumi M., Kanda N., Hayama K., Michimura Y., Miyoki S., Yamamoto T., Yusurihara H.

    Meeting abstracts of the Physical Society of Japan   67 ( 2 )   98 - 98   2012.08( ISSN:1342-8349

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  • スペース重力波アンテナDECIGO計画(36):DECIGO/DPF Reviewed

    安東正樹, 川村静児, 川村静児, 瀬戸直樹, 中村卓史, 坪野公夫, 佐藤修一, 田中貴浩, 船木一幸, 沼田健司, 神田展行, 井岡邦仁, 高島健, 横山順一, 青柳巧介, 我妻一博, 阿久津智忠, 浅田秀樹, 麻生洋一, 新井宏二, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 和泉究, 市來淨與, 伊東宏之, 伊藤洋介, 井上開輝, 上田暁俊, 植田憲一, 歌島昌由, 江口智士, 江尻悠美子, 榎基宏, 戎崎俊一, 江里口良治, 大石奈緒子

    日本物理学会講演概要集   67 ( 1 )   2012( ISSN:1342-8349

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    J-GLOBAL

  • スペース重力波アンテナDECIGO計画(21) Reviewed

    阿久津智忠, 安東正樹, 瀬戸直樹, 川村静児, 中村卓史, 坪野公夫, 佐藤修一, 田中貴浩, 船木一幸, 沼田健司, 神田展行, 井岡邦仁, 高島健, 横山順一, 青柳巧介, 我妻一博, 浅田秀樹, 麻生洋一, 新井宏二, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 和泉究, 市來淨與, 伊東宏之, 伊藤洋介, 井上開輝, 上田暁俊, 植田憲一, 歌島昌由, 江口智士, 榎基宏, 戎崎俊一, 江里口良治, 大石奈緒子, 大石奈緒子, 大河正志

    日本天文学会年会講演予稿集   2012   2012( ISSN:1347-0639

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    J-GLOBAL

  • 28aGS-1 Space Gravitational Wave Antenna DECIGO (30) : Design, Project Reviewed

    Kawamura Seiji

    Meeting abstracts of the Physical Society of Japan   66 ( 1 )   124 - 124   2011.03( ISSN:1342-8349

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  • 重力波とブラックホールの深い関係 Invited

    神田展行

    岩波書店・雑誌『科学』   ( 4 )   2011

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  • 重力波とブラックホールの深い関係 Reviewed

    神田展行

    岩波書店・雑誌『科学』   ( 4 )   2011

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  • 重力波とブラックホールの深い関係 Invited

    神田展行

    岩波書店・雑誌『科学』   ( 4 )   2011

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  • スペース重力波アンテナDECIGO計画(18):設計・計画・サイエンス Reviewed

    阿久津智忠, 川村静児, 川村静児, 安東正樹, 瀬戸直樹, 佐藤修一, 中村卓史, 坪野公夫, 船木一幸, 横山順一, 神田展行, 田中貴浩, 沼田健司, 高島健, 井岡邦仁, 青柳巧介, 我妻一博, 浅田秀樹, 麻生洋一, 新井宏二, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 和泉究, 市來淨與, 伊東宏之, 伊藤洋介, 井上開輝, 上田暁俊, 植田憲一, 歌島昌由, 江尻悠美子, 榎基宏, 戎崎俊一, 江里口良治, 大石奈緒子, 大石奈緒子

    日本天文学会年会講演予稿集   2011   2011( ISSN:1347-0639

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  • 13pSH-1 Space Gravitational Wave Antenna DECIGO (27) : Design, Project Reviewed

    Kawamura Seiji

    Meeting abstracts of the Physical Society of Japan   65 ( 2 )   91 - 91   2010.08( ISSN:1342-8349

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  • BI-1-7 Space gravitational wave detector : DECIGO & DPF Reviewed

    Sun Ke-Xun, Musha Mitsuru

    Proceedings of the IEICE General Conference   2010 ( 1 )   SS_85 - SS-86   2010.03( ISSN:1349-1369

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  • 21aBH-1 Space Gravitational Wave Antenna DECIGO (24) : Design, Project Reviewed

    Kawamura Seiji

    The Physical Society of Japan (JPS), Meeting Abstracts of the Physical Society of Japan   65 ( 0 )   2010( ISSN:1342-8349

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  • 21pBL-7 重力波検出器の現状と将来計画(21pBL 宇宙線・宇宙物理領域シンポジウム:一般相対論の直接検証:ブラックホール・シャドーの直接撮像と重力波の検出,宇宙線・宇宙物理領域) Reviewed

    神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集   65   2010

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    DOI: 10.11316/jpsgaiyo.65.1.1.0_116_2

  • 21pBL-7 重力波検出器の現状と将来計画(21pBL 宇宙線・宇宙物理領域シンポジウム:一般相対論の直接検証:ブラックホール・シャドーの直接撮像と重力波の検出,宇宙線・宇宙物理領域) Reviewed

    神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集   65 ( 0 )   116   2010( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.65.1.1.0_116_2

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  • 21aBH-1 Space Gravitational Wave Antenna DECIGO (24) : Design, Project

    Kawamura Seiji

    Meeting Abstracts of the Physical Society of Japan   65 ( 0 )   108 - 108   2010( ISSN:1342-8349

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  • 10aSE-4 Space Gravitational Wave Antenna DECIGO (20) : Design, Project Reviewed

    Kawamura Seiji

    Meeting abstracts of the Physical Society of Japan   64 ( 2 )   32 - 32   2009.08( ISSN:1342-8349

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  • DECIGO: The Japanese space gravitational wave antenna Reviewed

    Shuichi Sato, Seiji Kawamura, Masaki Ando, Takashi Nakamura, Kimio Tsubono, Akito Araya, Ikkoh Funaki, Kunihito Ioka, Nobuyuki Kanda, Shigenori Moriwaki, Mitsuru Musha, Kazuhiro Nakazawa, Kenji Numata, Shin Ichiro Sakai, Naoki Seto, Takeshi Takashima, Takahiro Tanaka, Kazuhiro Agatsuma, Koh Suke Aoyanagi, Koji Arai, Hideki Asada, Yoichi Aso, Takeshi Chiba, Toshikazu Ebisuzaki, Yumiko Ejiri, Motohiro Enoki, Yoshiharu Eriguchi, Masa Katsu Fujimoto, Ryuichi Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Katsuhiko Ganzu, Tomohiro Harada, Tatsuaki Hashimoto, Kazuhiro Hayama, Wataru Hikida, Yoshiaki Himemoto, Hisashi Hirabayashi, Takashi Hiramatsu, Feng Lei Hong, Hideyuki Horisawa, Mizuhiko Hosokawa, Kiyotomo Ichiki, Takeshi Ikegami, Kaiki TInoue, Koji Ishidoshiro, Hideki Ishihara, Takehiko Ishikawa, Hideharu Ishizaki, Hiroyuki Ito, Yousuke Itoh, Nobuki Kawashima, Fumiko Kawazoe, Kishimoto Naoko, Kenta Kiuchi, Shiho Kobayashi, Kazunori Kohri, Hiroyuki Koizumi, Yasufumi Kojima, Keiko Kokeyama, Wataru Kokuyama, Kei Kotake, Yoshihide Kozai, Hideaki Kudoh, Hiroo Kunimori, Hitoshi Kuninaka, Kazuaki Kuroda, Kei Ichi Maeda, Hideo Matsuhara, Yasushi Mino, Osamu Miyakawa, Shinji Miyoki, Mutsuko YMorimoto, Tomoko Morioka, Toshiyuki Morisawa, Shinji Mukohyama, Shigeo Nagano, Isao Naito, Kouji Nakamura, Hiroyuki Nakano, Kenichi Nakao, Shinichi Nakasuka, Yoshinori Nakayama, Erina Nishida, Kazutaka Nishiyama, Atsushi Nishizawa, Yoshito Niwa, Taiga Noumi, Yoshiyuki Obuchi, Masatake Ohashi, Naoko Ohishi, Masashi Ohkawa, Norio Okada, Kouji Onozato, Kenichi Oohara, Norichika Sago, Motoyuki Saijo, Masaaki Sakagami, Shihori Sakata, Misao Sasaki

    Journal of Physics: Conference Series   154   2009.06( ISSN:1742-6588

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    DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a differential Fabry-Perot interferometer. We plan to launch DECIGO in middle of 2020s, after sequence of two precursor satellite missions, DECIGO pathfinder and Pre-DECIGO, for technology demonstration required to realize DECIGO and hopefully for detection of gravitational waves from our galaxy or nearby galaxies. © 2009 IOP Publishing Ltd.

    DOI: 10.1088/1742-6596/154/1/012040

  • 29pXD-2 LCGT Project : Test of General Relativity and Astronomical Observation by Gravitational waves Reviewed

    Kuroda K, Nakatani I, Ohashi M, Fujimoto M-K, Kawamura S, Suzuki T, Saito Y, Tsubono K, Mio N, Araya A, Nakamura T, Ando M, Kanda N, LCGT Collaboration

    Meeting abstracts of the Physical Society of Japan   64 ( 1 )   97 - 97   2009.03( ISSN:1342-8349

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  • 30pSC-1 Space Gravitational Wave Antenna DECIGO (17) : Design, Project Reviewed

    Kawamura Seiji

    Meeting abstracts of the Physical Society of Japan   64 ( 1 )   100 - 100   2009.03( ISSN:1342-8349

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  • スペース重力波アンテナDECIGO計画(13) Reviewed

    川村静児, 安東正樹, 瀬戸直樹, 佐藤修一, 中村卓史, 坪野公夫, 船木一幸, 沼田健司, 神田展行, 田中貴浩, 井岡邦仁, 高島健, 青柳巧介, 我妻一博, 浅田秀樹, 麻生洋一, 新井宏二, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 市來淨與, 伊東宏之, 伊藤洋介, 井上開輝, 上田暁俊, 植田憲一, 歌島昌由, 江尻悠美子, 榎基宏, 戎崎俊一, 江里口良治, 大石奈緒子, 大河正志, 大橋正健, 大原謙一, 大渕喜之, 岡田健志

    日本天文学会年会講演予稿集   2009   2009( ISSN:1347-0639

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  • スペース重力波アンテナDECIGO計画(11) Reviewed

    川村静児, 安東正樹, 佐藤修一, 瀬戸直樹, 中村卓史, 坪野公夫, 船木一幸, 神田展行, 沼田健司, 田中貴浩, 井岡邦仁, 高島健, 青柳巧介, 我妻一博, 浅田秀樹, 麻生洋一, 新井宏二, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 市來淨興, 伊東宏之, 伊藤洋介, 井上開輝, 上田暁俊, 植田憲一, 歌島昌由, 江尻悠美子, 榎基広, 戎崎俊一, 江里口良治, 大石奈緒子, 大河正志, 大橋正健, 大原謙一, 大渕喜之, 岡田則夫

    日本天文学会年会講演予稿集   2009   2009( ISSN:1347-0639

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  • 23aSF-1 Space Gravitational Wave Antenna DECIGO XV : Overview, Roadmap, Path Finder Reviewed

    Ando M., Kawamura S., Seto N., Tanaka T., Nakamura T., Tsubono K.

    Meeting abstracts of the Physical Society of Japan   63 ( 2 )   91 - 91   2008.08( ISSN:1342-8349

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  • 24pZW-2 干渉計型重力波検出器TAMA300開発の現状XX(干渉計開発)(重力波,宇宙線・宇宙物理領域) Reviewed

    新井 宏二, 石崎 秀晴, 中川 憲保, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 辰巳 大輔, 安東 正樹, 三代木 伸二, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 高橋 竜太郎, 坪野 公夫, TAMA Conaboration, 和泉 究, 我妻 一博, 荒瀬 勇太, 若林 野花, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   63 ( 0 )   2008

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    DOI: 10.11316/jpsgaiyo.63.1.1.0_112_1

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  • The Japanese space gravitational wave antenna - DECIGO Reviewed

    S. Kawamura, M. Ando, T. Nakamura, K. Tsubono, T. Tanaka, I. Funaki, N. Seto, K. Numata, S. Sato, K. Ioka, N. Kanda, T. Takashima, K. Agatsuma, T. Akutsu, T. Akutsu, K.-S. Aoyanagi, K. Arai, Y. Arase, A. Araya, H. Asada, Y. Aso, T. Chiba, T. Ebisuzaki, M. Enoki, Y. Eriguchi, M.-K. Fujimoto, R. Fujita, M. Fukushima, T. Futamase, K. Ganzu, T. Harada, T. Hashimoto, K. Hayama, W. Hikida, Y. Himemoto, H. Hirabayashi, T. Hiramatsu, F.-L. Hong, H. Horisawa, M. Hosokawa, K. Ichiki, T. Ikegami, K.T. Inoue, K. Ishidoshiro, H. Ishihara, T. Ishikawa, H. Ishizaki, H. Ito, Y. Itoh, S. Kamagasako, N. Kawashima, F. Kawazoe, H. Kirihara, N. Kishimoto, K. Kiuchi, S. Kobayashi, K. Kohri, H. Koizumi, Y. Kojima, K. Kokeyama, W. Kokuyama, K. Kotake, Y. Kozai, H. Kudoh, H. Kunimori, H. Kuninaka, K. Kuroda, K.-I. Maeda, H. Matsuhara, Y. Mino, O. Miyakawa, S. Miyoki, Y. Morimoto, T. Morioka, T. Morisawa, S. Moriwaki, S. Mukohyama, M. Musha, S. Nagano, I. Naito, N. Nakagawa, K. Nakamura, H. Nakano, K. Nakao, S. Nakasuka, Y. Nakayama, E. Nishida, K. Nishiyama, A. Nishizawa, Y. Niwa, M. Ohashi, N. Ohishi, M. Ohkawa, A. Okutomi, K. Onozato, K. Oohara, N. Sago, M. Saijo, M. Sakagami, S.-I. Sakai, S. Sakata, M. Sasaki, T. Sato, M. Shibata, H. Shinkai, K. Somiya, H. Sotani, N. Sugiyama, Y. Suwa, H. Tagoshi, K. Takahashi, K. Takahashi, T. Takahashi, H. Takahashi, R. Takahashi, R. Takahashi, A. Takamori, T. Takano, K. Taniguchi, A. Taruya, H. Tashiro, M. Tokuda, M. Tokunari, M. Toyoshima, S. Tsujikawa, Y. Tsunesada, K.-I. Ueda, M. Utashima, H. Yamakawa, K. Yamamoto, T. Yamazaki, J. Yokoyama, C.-M. Yoo, S. Yoshida, T. Yoshino

    Journal of Physics: Conference Series   122   2008

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    DOI: 10.1088/1742-6596/122/1/012006

  • スペース重力波アンテナDECIGO計画(9) Reviewed

    川村静児, 安東正樹, 中村卓史, 坪野公夫, 田中貴浩, 船木一幸, 瀬戸直樹, 沼田健司, 佐藤修一, 神田展行, 井岡邦仁, 高島健, 青柳巧介, 我妻一博, 阿久津智忠, 阿久津朋美, 浅田秀樹, 麻生洋一, 新井宏二, 荒瀬勇太, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 市來浄與, 伊東宏之, 伊藤洋介, 井上開輝, 植田憲一, 歌島昌由, 榎基宏, 戎崎俊一, 江里口良治, 大石奈緒子, 大河正志, 大橋正健, 大原謙一, 奥冨聡

    日本天文学会年会講演予稿集   2008   2008( ISSN:1347-0639

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  • 24pZW-2 干渉計型重力波検出器TAMA300開発の現状XX(干渉計開発)(重力波,宇宙線・宇宙物理領域) Reviewed

    新井 宏二, 石崎 秀晴, 中川 憲保, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 辰巳 大輔, 安東 正樹, 三代木 伸二, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 高橋 竜太郎, 坪野 公夫, TAMA Conaboration, 和泉 究, 我妻 一博, 荒瀬 勇太, 若林 野花, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集   63 ( 0 )   112 - 112   2008( ISSN:1342-8349 ( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.63.1.1.0_112_1

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  • 21aZH-1 Space Gravitational Wave Antenna DECIGO X (Design, Project) Reviewed

    Kawamura Seiji

    Meeting abstracts of the Physical Society of Japan   62 ( 2 )   95 - 95   2007.08( ISSN:1342-8349

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  • 21aZH-3 Space Gravitational Wave Antenna DECIGO XI (Science) Reviewed

    Seto Naoki

    Meeting abstracts of the Physical Society of Japan   62 ( 2 )   96 - 96   2007.08( ISSN:1342-8349

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  • 28pSG-5 The effect of the cosmic rays on the interferometeric gravitational wave detector Reviewed

    Yamamoto K., Okada A., Uchiyama T., Miyoki S., Ohashi M., Kuroda K., Hayakawa H., Kanda N., Tatsumi D., Tsunesada Y.

    Meeting abstracts of the Physical Society of Japan   62 ( 1 )   113 - 113   2007.02( ISSN:1342-8349

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  • 21pZH-2 干渉計型重力波検出器TAMA300開発の現状 XV : 低周波防振装置2(21pZH 重力波,宇宙線・宇宙物理領域) Reviewed

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 高橋 竜太郎, 森脇 成典, 神田 履行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴, 新井 宏二, 辰巳 大輔, 和泉 究

    一般社団法人 日本物理学会 日本物理学会講演概要集   62   2007

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    DOI: 10.11316/jpsgaiyo.62.2.1.0_99_2

  • 21pZH-2 干渉計型重力波検出器TAMA300開発の現状 XV : 低周波防振装置2(21pZH 重力波,宇宙線・宇宙物理領域) Reviewed

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 高橋 竜太郎, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴, 新井 宏二, 辰巳 大輔, 和泉 究

    一般社団法人 日本物理学会 日本物理学会講演概要集   62 ( 0 )   99   2007( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.62.2.1.0_99_2

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  • スペース重力波アンテナDECIGO計画(8) Reviewed

    川村静児, 安東正樹, 瀬戸直樹, 中村卓史, 坪野公夫, 田中貴浩, 船木一幸, 沼田健司, 佐藤修一, 神田展行, 高島健, 井岡邦仁, 青柳巧介, 我妻一博, 阿久津智忠, 阿久津朋美, 浅田秀樹, 麻生洋一, 新井宏二, 荒瀬勇太, 新谷昌人, 池上健, 石川毅彦, 石崎秀晴, 石徹白晃治, 石原秀樹, 市來浄輿, 伊東宏之, 伊藤洋介, 井上開輝, 植田憲一, 歌島昌由, 榎基宏, 戎崎俊一, 江里口良治, 大石奈緒子, 大河正志, 大橋正健, 大原謙一, 奥冨聡

    日本天文学会年会講演予稿集   2007   2007( ISSN:1347-0639

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  • 20pSG-5 Evaluation of GCC statistics by using TAMA300 data Reviewed

    ISHIDOSHIRO Koji, HIMEMOTO Yoshiaki, KANDA Nobuyuki, ANDO Masaki, TSUBONO Kimio

    Meeting abstracts of the Physical Society of Japan   61 ( 2 )   57 - 57   2006.08( ISSN:1342-8349

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  • 27aTG-7 Analysis of TAMA300 data for burst gravitational waves using ALF filter Reviewed

    Akutsu T, Ando M, Kanda N, Tatsumi D, Telada S, Miyoki S, Ohashi M, TAMA Collaboration

    Meeting abstracts of the Physical Society of Japan   61 ( 1 )   86 - 86   2006.03( ISSN:1342-8349

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  • 28pTG-11 Digital feedback control of interferometer with DSP Reviewed

    Awaya N., Tokuda M., Honda R., Kanda N.

    Meeting abstracts of the Physical Society of Japan   61 ( 1 )   101 - 101   2006.03( ISSN:1342-8349

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  • 27aTG-8 Burst GW search with TAMA300 data using multivariate cluster Reviewed

    Honda R, Ando M, Tagoshi H, Tatsumi D, Awaya N, Tokuda M, Kanda N

    Meeting abstracts of the Physical Society of Japan   61 ( 1 )   86 - 86   2006.03( ISSN:1342-8349

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  • 26pXH-2 Current states of Burst analysis of TAMA 300 data with the ALF filter Reviewed

    Akutsu T., Ando M., Kanda N., Tatsumi D., Telada S., Hayakawa H., Yamamoto K., Miyoki S., Ohashi M., Kuroda K.

    Meeting abstracts of the Physical Society of Japan   60 ( 1 )   96 - 96   2005.03( ISSN:1342-8349

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  • 27aXH-5 Study for Correlation Analysis Cross Talk between two LCGT interferometer signal Reviewed

    Kanda N., Takahashi H., Tagoshi H., Sago N., Tatsumi D., Tsunesada Y., Ando M., LCGT collaboration

    Meeting abstracts of the Physical Society of Japan   60 ( 1 )   101 - 101   2005.03( ISSN:1342-8349

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  • 26pXH-4 Result of search for gravitational waves from black hole ringing in TAMA300 data Reviewed

    Tsunesada Y., Kanda N., Nakano H., Tatsumi D., The TAMA Collaboration

    Meeting abstracts of the Physical Society of Japan   60 ( 1 )   97 - 97   2005.03( ISSN:1342-8349

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  • 15aSF-4 TAMA300データを用いたバースト重力波解析V(15aSF 重力波,宇宙線・宇宙物理領域) Reviewed

    安東 正樹, 三尾 典克, 三代木 伸二, 森脇 成典, 長野 重夫, 佐藤 修一, 柴田 大, 田越 秀行, 高橋 弘毅, 高橋 竜太郎, 辰巳 大輔, 阿久津 朋美, 常定 芳基, 山崎 利孝, 他TAMA Collaboration, 阿久津 智忠, 新井 宏二, 麻生 洋一, 福嶋 美津広, 端山 和大, 神田 展行, 近藤 寿浩

    一般社団法人 日本物理学会 日本物理学会講演概要集   60 ( 0 )   2005

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    DOI: 10.11316/jpsgaiyo.60.2.1.0_37_4

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  • 15aSF-4 TAMA300データを用いたバースト重力波解析V(15aSF 重力波,宇宙線・宇宙物理領域) Reviewed

    安東 正樹, 三尾 典克, 三代木 伸二, 森脇 成典, 長野 重夫, 佐藤 修一, 柴田 大, 田越 秀行, 高橋 弘毅, 高橋 竜太郎, 辰巳 大輔, 阿久津 朋美, 常定 芳基, 山崎 利孝, 他TAMA Collaboration, 阿久津 智忠, 新井 宏二, 麻生 洋一, 福嶋 美津広, 端山 和大, 神田 展行, 近藤 寿浩

    一般社団法人 日本物理学会 日本物理学会講演概要集   60 ( 0 )   37 - 37   2005( ISSN:1342-8349 ( eISSN:21890803

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    DOI: 10.11316/jpsgaiyo.60.2.1.0_37_4

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  • Education of Physics Experiment using Michelson Interferometer System

    Nobuyuki Kanda, Yoshiaki Chiba, Misako Ikehata, Yasuo Ishiguro, Mayu Katsuki

    27 ( 1 )   85   2003

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  • Observation Target and Data Analysis of Laser Interferometric Gravitational Wave Detector

    94 ( 10 )   448 - 456   2001

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Presentations

  • 時空の歪みの伝播、重力波で探る宇宙 Invited Domestic conference

    神田展行

    第9回オンライン物理講話  2022.06 

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    Presentation type:Public lecture, seminar, tutorial, course, or other speech  

  • 重力波の初観測から現状 Invited Domestic conference

    神田展行, KAGRAコラボレーション

    ELPHシンポジウム2022―2021年度電子光理学研究拠点共同利用成果報告会  2022.03 

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    Presentation type:Oral presentation (general)  

  • Future Prospects of KAGRA gravitational wave observation on Multi-messenger astronomy Domestic conference

    Nobuyuki Kanda, KAGRA collaboration

    Future Prospects of KAGRA gravitational wave observation on Multi-messenger astronomy  2021.09 

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  • Future Prospects of KAGRA gravitational wave observation on Multi-messenger astronomy Invited Domestic conference

    Nobuyuki Kanda, KAGRA collaboration

    2021.09 

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    Presentation type:Oral presentation (invited, special)  

  • Status of KAGRA Domestic conference

    Nobuyuki Kanda, on behalf of, KAGRA collaboration

    The 14th International Conference on Gravitation, Astrophysics and Cosmology (ICGAC14)  2020.08 

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  • Status of KAGRA Invited Domestic conference

    Nobuyuki Kanda, on behalf of, KAGRA collaboration

    The 14th International Conference on Gravitation, Astrophysics and Cosmology (ICGAC14)  2020.08 

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    Presentation type:Oral presentation (invited, special)  

  • KAGRAデータ転送・保管系の観測運転に向けた構築と整備 Domestic conference

    神田展行、KAGRA collaboration

    日本物理学会 2019年秋季大会  2019.09 

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    Presentation type:Oral presentation (general)  

  • KAGRAデータ転送・保管系の観測運転に向けた構築と整備 Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 2019年秋季大会  2019.09 

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  • KAGRAデータ転送・保管系の観測運転に向けた構築と整備 Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 2019年秋季大会  2019.09 

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  • KAGRA Data Tier International conference

    Nobuyuki Kanda, on behalf of the KAGRA collaboration

    16th International Conference on Topics in Astroparticle and Underground Physics  2019.09 

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  • KAGRA Data Tier Domestic conference

    Nobuyuki Kanda, on behalf of, the, KAGRA collaboration

    16th International Conference on Topics in Astroparticle and Underground Physics  2019.09 

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    Presentation type:Oral presentation (general)  

  • KAGRA Data Tier International conference

    Nobuyuki Kanda, on behalf of, the, KAGRA collaboration

    16th International Conference on Topics in Astroparticle and Underground Physics  2019.09 

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    Presentation type:Oral presentation (general)  

  • KAGRAのデータ配送と国際重力波観測ネットワークのデータ共有 Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 第74回年次大会  2019.03 

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    Presentation type:Oral presentation (general)  

  • KAGRAのデータ配送と国際重力波観測ネットワークのデータ共有 Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 第74回年次大会  2019.03 

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  • KAGRAのデータ配送と国際重力波観測ネットワークのデータ共有 Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 第74回年次大会  2019.03 

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  • Status of KAGRA toward the observation in 2019-2020 Invited International conference

    Nobuyuki Kanda, on behalf of KAGRA collaboration

    Status of KAGRA toward the observation in 2019-2020  2018.10 

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  • Status of KAGRA toward the observation in 2019-2020 Domestic conference

    Nobuyuki Kanda, on behalf of, KAGRA collaboration

    Status of KAGRA toward the observation in 2019-2020  2018.10 

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  • Status of KAGRA toward the observation in 2019-2020 Invited International conference

    Nobuyuki Kanda, on behalf of, KAGRA collaboration

    Status of KAGRA toward the observation in 2019-2020  2018.10 

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  • キャリブレーションの系統誤差効果を考慮したKAGRAシミュレーションデータ Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 2018年秋季大会  2018.10 

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  • キャリブレーションの系統誤差効果を考慮したKAGRAシミュレーションデータ Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 2018年秋季大会  2018.10 

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  • キャリブレーションの系統誤差効果を考慮したKAGRAシミュレーションデータ Domestic conference

    神田展行, KAGRA collaboration

    日本物理学会 2018年秋季大会  2018.10 

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  • Status of KAGRA Invited International conference

    Nobuyuki Kanda (Osaka City U.) on behalf of the KAGRA collaboration

    LSC-Virgo Meeting  2018.09 

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  • Status of KAGRA Domestic conference

    Nobuyuki Kanda, Osaka City, on behalf of, the, KAGRA collaboration

    LSC-Virgo Meeting  2018.09 

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  • Status of KAGRA Invited International conference

    Nobuyuki Kanda, Osaka City, on behalf of, the, KAGRA collaboration

    LSC-Virgo Meeting  2018.09 

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  • Subsystem report : DMG(2) Domestic conference

    N.Kanda

    20th KAGRA face-to-face meeting  2018.08 

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  • Subsystem report : DMG(2) Domestic conference

    N.Kanda

    20th KAGRA face-to-face meeting  2018.08 

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  • Subsystem report : DMG(2) Domestic conference

    N.Kanda

    20th KAGRA face-to-face meeting  2018.08 

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  • KAGRA data management : Toward Phase-II and O3 International conference

    N.Kanda on behalf of KAGRA collaboration

    4th KAGRA international workshop  2018.06 

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  • KAGRA data management : Toward Phase-II and O3 Domestic conference

    N.Kanda on, ehalf of, KAGRA collaboration

    4th KAGRA international workshop  2018.06 

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  • KAGRA data management : Toward Phase-II and O3 International conference

    N.Kanda on, ehalf of, KAGRA collaboration

    4th KAGRA international workshop  2018.06 

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  • DMG subsystem report (2): Toward Phase-II and O3 Domestic conference

    N.Kanda

    19th KAGRA face-to-face Meeting  2018.05 

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  • DMG subsystem report (2): Toward Phase-II and O3 Domestic conference

    N.Kanda

    19th KAGRA face-to-face Meeting  2018.05 

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  • DMG subsystem report (2): Toward Phase-II and O3 Domestic conference

    N.Kanda

    19th KAGRA face-to-face Meeting  2018.05 

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  • 重力波観測でわかる連星合体の姿 Domestic conference

    神田展行

    日本天文学会  2018.03 

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  • 重力波観測でわかる連星合体の姿 Invited Domestic conference

    神田展行

    日本天文学会  2018.03 

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  • 重力波観測でわかる連星合体の姿 Invited Domestic conference

    神田展行

    日本天文学会  2018.03 

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  • Overview of this workshop GWASNe2018 and (personal) prospect for GW detection/analysis for CCSN Invited International conference

    Nobuyuki Kanda

    Overview of this workshop GWASNe2018 and (personal) prospect for GW detection/analysis for CCSN  2018.02 

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  • Overview of this workshop GWASNe2018 and (personal) prospect for GW detection/analysis for CCSN Domestic conference

    Nobuyuki Kanda

    Overview of this workshop GWASNe2018 and (personal) prospect for GW detection/analysis for CCSN  2018.02 

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  • Overview of this workshop GWASNe2018 and (personal) prospect for GW detection/analysis for CCSN Invited International conference

    Nobuyuki Kanda

    Overview of this workshop GWASNe2018 and (personal) prospect for GW detection/analysis for CCSN  2018.02 

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  • (シンポジウム講演)「重力波実験の現状と展望」 Domestic conference

    神田展行

    日本物理学会  2017.09 

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  • (シンポジウム講演)「重力波実験の現状と展望」 Invited Domestic conference

    神田展行

    日本物理学会  2017.09 

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  • (シンポジウム講演)「重力波実験の現状と展望」 Invited Domestic conference

    神田展行

    日本物理学会  2017.09 

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  • 22pDJ-13 神岡におけるシューマン共振の測定 Domestic conference

    熱田 将, 齊藤 芳男, 宗宮 健太郎, 西澤 篤志, 宮川 治, 三代木 伸二, 矢野 和城, 小河 勉, 山口 覚, 端山 和大, 新谷 昌人, 上嶋 誠, 内山 隆, 小野 謙次, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集  2015 

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  • 22pDJ-13 神岡におけるシューマン共振の測定 Domestic conference

    熱田 将, 齊藤 芳男, 宗宮 健太郎, 西澤 篤志, 宮川 治, 三代木 伸二, 矢野 和城, 小河 勉, 山口 覚, 端山 和大, 新谷 昌人, 上嶋 誠, 内山 隆, 小野 謙次, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集  2015 

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  • 20aSB-1 大型低温重力波望遠鏡(KAGRA)プロジェクトの現状(20aSB 重力波(KAGRA),宇宙線・宇宙物理領域) Domestic conference

    麻生 洋一, 梶田 隆章, 黒田 和明, 大橋 正健, 川村 静児, 三代木 伸二, 内山 隆, 宮川 治, 齋藤 芳男, 大石 奈緒子, 山元 一広, Khalaidovski Alexandar, Kumar Rahul, 大嶋 新一, 石塚 秀喜, 廣瀬 榮一, 上泉 眞裕, 榊原 裕介, 関口 貴令, 陳 タン, 中野 雅之, 小野 謙次, 小仁所 志栞, 西村 翼, 渡辺 篤, 山中 祐治, 宮本 昴拓, 田中 宏樹, 藤本 眞克, Flaminio Raffaele, 高橋 竜太郎, 上田 暁俊, 阿久津 智忠, 辰巳 大輔, 中村 康二, Arellano Fabian Pena, 石崎 秀晴, 鳥居 泰男, 田中 伸幸, 山本 明, 鈴木 敏一, 木村 誠宏, 都丸 隆行, 井岡 邦仁, 久米 達哉, 小池 重明, 横山 順一, 伊藤 洋介, 枝 和成, 坪野 公夫, 安東 正樹, 平松 成範, 穀山 渉, 岡田 健志, 松本 伸之, 道村 唯太, 正田 亜八香, 柴田 和憲, 牛場 崇文, 渡部 恭平, 三尾 典克, 大前 宣昭, 鈴木 健一郎, 古谷 寛之, 細谷 暁夫, 河合 誠之, 宗宮 健太郎, 須佐 友紀, 上田 慎一郎, 加藤 準平, 粂田 綾香, 神田 展行, 端山 和大, 横澤 孝章, 山本 尚弘, 譲原 浩貴, 田中 一幸, 浅野 光洋, 鳥谷 仁人, 有馬 司, 宮本 晃伸, 中尾 憲一, 中村 卓史, 田中 貴浩, 瀬戸 直樹, 西澤 篤志, 植田 憲一, 米田 仁紀, 中川 賢一, 武者 満, 新谷 昌人, 高森 昭光, 佐藤 修一, 林 翔平, 奥富 弘基, 高辻 利之, 尾藤 洋一, 寺田 聡一, 長野 重夫, 田越 秀行, 上野 昂, 成川 達也, 佐野 保道, 高倉 理, Baiotti Luca, 佐々木 節, 柴田 大, 樽家 篤史, 中野 寛之, 関口 雄一郎, 佐合 紀親, 斎藤 那菜, 新冨 孝和, 大原 謙一, 金山 雅人, 若松 剛司, 佐藤 孝, 大河 正志, 土井 康平, 齊藤 高大, 飯島 音浩, 志賀 和成, 高橋 弘毅, 姫本 宣朗, 浅田 秀樹, 二間瀬 敏史, 高橋 史宜, 原田 知広, 小嶌 康史, 瓜生 康史, 山田 章一, 西條 統之, 大森 隆夫, 松島 房和, 森脇 喜紀, 小林 かおり, 榎本 勝成, 大石 諒, 〓ノ下 陽哉, 柿崎 充, 小野 行徳, 堀 匡寛, 早川 陽介, 廣林 茂樹, 沖野 浩二, Ruggero Micheletto, 固武 慶, 江口 智士, 中谷 一郎, 阪田 紫帆里, 鹿野 豊, 春山 富義, 上原 知幸, 川添 史子, Chen Yanbei, 河邉 径太, 新井 宏二, Miao Haixing, 和泉 究, Tobar M.E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, 苔山 圭以子, Zhu Zong-Hong, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, 沼田 健司, Marka Szabolcs, Marka Zsuzsanna, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Matta Vincenzo, Postiglione Fabio, Longo Maurizio, Addesso Paolo, Fusco Adele, Majorana Ettore, Zhai Xiang-hua, Xi Ping, Ni Wei-Tou, Mei Hsien-Hao, Yoon Tai Hyun, Lee Hyung Won, Kim Kyoung Yee, Kim Jeongcho, Lee Hyung Mok, Kim Chunglee, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, van Putten, Maurice H.P.M, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya, 樫山 和己, 八木 絢外, Pai Archana, 我妻 一博, 久徳 浩太郎

    日本物理学会講演概要集  2014.08  一般社団法人日本物理学会

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  • 20aSB-1 大型低温重力波望遠鏡(KAGRA)プロジェクトの現状(20aSB 重力波(KAGRA),宇宙線・宇宙物理領域) Domestic conference

    麻生 洋一, 梶田 隆章, 黒田 和明, 大橋 正健, 川村 静児, 三代木 伸二, 内山 隆, 宮川 治, 齋藤 芳男, 大石 奈緒子, 山元 一広, Khalaidovski Alexandar, Kumar Rahul, 大嶋 新一, 石塚 秀喜, 廣瀬 榮一, 上泉 眞裕, 榊原 裕介, 関口 貴令, 陳 タン, 中野 雅之, 小野 謙次, 小仁所 志栞, 西村 翼, 渡辺 篤, 山中 祐治, 宮本 昴拓, 田中 宏樹, 藤本 眞克, Flaminio Raffaele, 高橋 竜太郎, 上田 暁俊, 阿久津 智忠, 辰巳 大輔, 中村 康二, Arellano Fabian Pena, 石崎 秀晴, 鳥居 泰男, 田中 伸幸, 山本 明, 鈴木 敏一, 木村 誠宏, 都丸 隆行, 井岡 邦仁, 久米 達哉, 小池 重明, 横山 順一, 伊藤 洋介, 枝 和成, 坪野 公夫, 安東 正樹, 平松 成範, 穀山 渉, 岡田 健志, 松本 伸之, 道村 唯太, 正田 亜八香, 柴田 和憲, 牛場 崇文, 渡部 恭平, 三尾 典克, 大前 宣昭, 鈴木 健一郎, 古谷 寛之, 細谷 暁夫, 河合 誠之, 宗宮 健太郎, 須佐 友紀, 上田 慎一郎, 加藤 準平, 粂田 綾香, 神田 展行, 端山 和大, 横澤 孝章, 山本 尚弘, 譲原 浩貴, 田中 一幸, 浅野 光洋, 鳥谷 仁人, 有馬 司, 宮本 晃伸, 中尾 憲一, 中村 卓史, 田中 貴浩, 瀬戸 直樹, 西澤 篤志, 植田 憲一, 米田 仁紀, 中川 賢一, 武者 満, 新谷 昌人, 高森 昭光, 佐藤 修一, 林 翔平, 奥富 弘基, 高辻 利之, 尾藤 洋一, 寺田 聡一, 長野 重夫, 田越 秀行, 上野 昂, 成川 達也, 佐野 保道, 高倉 理, Baiotti Luca, 佐々木 節, 柴田 大, 樽家 篤史, 中野 寛之, 関口 雄一郎, 佐合 紀親, 斎藤 那菜, 新冨 孝和, 大原 謙一, 金山 雅人, 若松 剛司, 佐藤 孝, 大河 正志, 土井 康平, 齊藤 高大, 飯島 音浩, 志賀 和成, 高橋 弘毅, 姫本 宣朗, 浅田 秀樹, 二間瀬 敏史, 高橋 史宜, 原田 知広, 小嶌 康史, 瓜生 康史, 山田 章一, 西條 統之, 大森 隆夫, 松島 房和, 森脇 喜紀, 小林 かおり, 榎本 勝成, 大石 諒, 〓ノ下 陽哉, 柿崎 充, 小野 行徳, 堀 匡寛, 早川 陽介, 廣林 茂樹, 沖野 浩二, Ruggero Micheletto, 固武 慶, 江口 智士, 中谷 一郎, 阪田 紫帆里, 鹿野 豊, 春山 富義, 上原 知幸, 川添 史子, Chen Yanbei, 河邉 径太, 新井 宏二, Miao Haixing, 和泉 究, Tobar M.E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, 苔山 圭以子, Zhu Zong-Hong, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, 沼田 健司, Marka Szabolcs, Marka Zsuzsanna, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Matta Vincenzo, Postiglione Fabio, Longo Maurizio, Addesso Paolo, Fusco Adele, Majorana Ettore, Zhai Xiang-hua, Xi Ping, Ni Wei-Tou, Mei Hsien-Hao, Yoon Tai Hyun, Lee Hyung Won, Kim Kyoung Yee, Kim Jeongcho, Lee Hyung Mok, Kim Chunglee, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, van Putten, Maurice H.P.M, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya, 樫山 和己, 八木 絢外, Pai Archana, 我妻 一博, 久徳 浩太郎

    日本物理学会講演概要集  2014.08  一般社団法人日本物理学会

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    Presentation type:Oral presentation (general)  

  • 27aTL-1 大型低温重力波望遠鏡(KAGRA)プロジェクトの現状(27aTL 重力波(KAGRA),宇宙線・宇宙物理領域) Domestic conference

    安東 正樹, 梶田 隆章, 黒田 和明, 大橋 正健, 川村 静児, 三代木 伸二, 内山 隆, 宮川 治, 大石 奈緒子, 山元 一広, Khalaidovski Alexandar, Kumar Rahul, 西田 恵里奈, 石塚 秀喜, 東谷 千比呂, 廣瀬 榮一, 上泉 眞裕, 岩崎 詩子, 榊原 裕介, 関口 貴令, 陳 タン, 中野 雅之, 手嶋 航大, 小野 謙次, 小仁所 志栞, 西村 翼, 渡辺 篤, 藤本 眞克, Flaminio Raffaele, 高橋 竜太郎, 上田 暁俊, 阿久津 智忠, 辰巳 大輔, 中村 康二, Arellano Fabian Pena, Friedrich Daniel, 石崎 秀晴, 鳥居 泰男, 田中 伸幸, 奥冨 弘基, 江口 智士, 山本 明, 鈴木 敏一, 木村 誠宏, 都丸 隆行, 井岡 邦仁, 齊藤 芳男, 久米 達哉, 小池 重明, 横山 順一, 樽家 篤史, 伊藤 洋介, 坪野 公夫, 麻生 洋一, 平松 成範, 穀山 渉, 岡田 健志, 松本 伸之, 道村 唯太, 正田 亜八香, 柴田 和憲, 牛場 崇文, 渡辺 恭平, 三尾 典克, 森脇 成典, 大前 宣昭, 千葉 智弘, 福本 展大, 鈴木 健一郎, 古谷 寛之, 細谷 暁夫, 河合 誠之, 宗宮 健太郎, 須佐 友紀, 上田 慎一郎, 加藤 準平, 粂田 綾香, 神田 展行, 端山 和大, 横澤 孝章, 山本 尚弘, 譲原 浩貴, 田中 一幸, 浅野 光洋, 鳥谷 仁人, 中尾 憲一, 中村 卓史, 瀬戸 直樹, 西澤 篤志, 植田 憲一, 米田 仁紀, 中川 賢一, 武者 満, 新谷 昌人, 高森 昭光, 佐藤 修一, 林 翔平, 東浦 孝典, 高辻 利之, 尾藤 洋一, 寺田 総一, 長野 重夫, 田越 秀行, 上野 昂, 成川 達也, 佐野 保道, 高倉 理, Baiotti Luca, 佐々木 節, 柴田 大, 田中 貴浩, 中野 寛之, 関口 雄一郎, 佐合 紀親, 斎藤 那菜, 新冨 孝和, 大原 謙一, 平沼 悠太, 金山 雅人, 若松 剛司, 佐藤 孝, 大河 正志, 土井 康平, 前原 進也, 清水 直弥, 高橋 弘毅, 姫本 宣朗, 浅田 秀樹, 二間瀬 敏史, 高橋 史宜, 原田 知広, 小嶌 康史, 瓜生 康史, 山田 章一, 西條 統之, 大森 隆夫, 松島 房和, 森脇 喜紀, 小林 かおり, 榎本 勝成, 米山 直弥, 宮本 達也, 大石 諒, 〓ノ下 陽哉, 柿崎 充, 小野 行徳, 堀 匡寛, 早川 陽介, 廣林 茂樹, 沖野 浩二, Ruggero Micheletto, 固武 慶, 中谷 一郎, 阪田 紫帆里, 鹿野 豊, 春山 富義, 上原 知幸, 川添 史子, Chen Yanbei, 河邉 径太, 新井 宏二, Miao Haixing, 和泉 究, Tobar M.E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, 苔山 圭以子, Zhu Zong-Hong, Dhurandhar S, Mitra S, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, 沼田 健司, Marka Szabolcs, Marka Zsuzsanna, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Matta Vincenzo, Postiglione Fabio, Longo Maurizio, Addesso Paolo, Fusco Adele, Majorana Ettore, Zhai Xiang-hua, Xi Ping, Ni Wei-Tou, Mei Hsien-Hao, Wu Shan-Jyun, Yoon Tai Hyun, Lee Hyung Won, Kim Kyoung Yee, Kim Jeongcho, Lee Hyung Mok, Kim Chunglee, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, Putten Maurice, H.P.M. van, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya, 樫山 和己, 八木 絢外, Pai Archana, 我妻 一博, 久徳 浩太郎

    日本物理学会講演概要集  2014.03  一般社団法人日本物理学会

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  • 27aTL-1 大型低温重力波望遠鏡(KAGRA)プロジェクトの現状(27aTL 重力波(KAGRA),宇宙線・宇宙物理領域) Domestic conference

    安東 正樹, 梶田 隆章, 黒田 和明, 大橋 正健, 川村 静児, 三代木 伸二, 内山 隆, 宮川 治, 大石 奈緒子, 山元 一広, Khalaidovski Alexandar, Kumar Rahul, 西田 恵里奈, 石塚 秀喜, 東谷 千比呂, 廣瀬 榮一, 上泉 眞裕, 岩崎 詩子, 榊原 裕介, 関口 貴令, 陳 タン, 中野 雅之, 手嶋 航大, 小野 謙次, 小仁所 志栞, 西村 翼, 渡辺 篤, 藤本 眞克, Flaminio Raffaele, 高橋 竜太郎, 上田 暁俊, 阿久津 智忠, 辰巳 大輔, 中村 康二, Arellano Fabian Pena, Friedrich Daniel, 石崎 秀晴, 鳥居 泰男, 田中 伸幸, 奥冨 弘基, 江口 智士, 山本 明, 鈴木 敏一, 木村 誠宏, 都丸 隆行, 井岡 邦仁, 齊藤 芳男, 久米 達哉, 小池 重明, 横山 順一, 樽家 篤史, 伊藤 洋介, 坪野 公夫, 麻生 洋一, 平松 成範, 穀山 渉, 岡田 健志, 松本 伸之, 道村 唯太, 正田 亜八香, 柴田 和憲, 牛場 崇文, 渡辺 恭平, 三尾 典克, 森脇 成典, 大前 宣昭, 千葉 智弘, 福本 展大, 鈴木 健一郎, 古谷 寛之, 細谷 暁夫, 河合 誠之, 宗宮 健太郎, 須佐 友紀, 上田 慎一郎, 加藤 準平, 粂田 綾香, 神田 展行, 端山 和大, 横澤 孝章, 山本 尚弘, 譲原 浩貴, 田中 一幸, 浅野 光洋, 鳥谷 仁人, 中尾 憲一, 中村 卓史, 瀬戸 直樹, 西澤 篤志, 植田 憲一, 米田 仁紀, 中川 賢一, 武者 満, 新谷 昌人, 高森 昭光, 佐藤 修一, 林 翔平, 東浦 孝典, 高辻 利之, 尾藤 洋一, 寺田 総一, 長野 重夫, 田越 秀行, 上野 昂, 成川 達也, 佐野 保道, 高倉 理, Baiotti Luca, 佐々木 節, 柴田 大, 田中 貴浩, 中野 寛之, 関口 雄一郎, 佐合 紀親, 斎藤 那菜, 新冨 孝和, 大原 謙一, 平沼 悠太, 金山 雅人, 若松 剛司, 佐藤 孝, 大河 正志, 土井 康平, 前原 進也, 清水 直弥, 高橋 弘毅, 姫本 宣朗, 浅田 秀樹, 二間瀬 敏史, 高橋 史宜, 原田 知広, 小嶌 康史, 瓜生 康史, 山田 章一, 西條 統之, 大森 隆夫, 松島 房和, 森脇 喜紀, 小林 かおり, 榎本 勝成, 米山 直弥, 宮本 達也, 大石 諒, 〓ノ下 陽哉, 柿崎 充, 小野 行徳, 堀 匡寛, 早川 陽介, 廣林 茂樹, 沖野 浩二, Ruggero Micheletto, 固武 慶, 中谷 一郎, 阪田 紫帆里, 鹿野 豊, 春山 富義, 上原 知幸, 川添 史子, Chen Yanbei, 河邉 径太, 新井 宏二, Miao Haixing, 和泉 究, Tobar M.E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, 苔山 圭以子, Zhu Zong-Hong, Dhurandhar S, Mitra S, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, 沼田 健司, Marka Szabolcs, Marka Zsuzsanna, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Matta Vincenzo, Postiglione Fabio, Longo Maurizio, Addesso Paolo, Fusco Adele, Majorana Ettore, Zhai Xiang-hua, Xi Ping, Ni Wei-Tou, Mei Hsien-Hao, Wu Shan-Jyun, Yoon Tai Hyun, Lee Hyung Won, Kim Kyoung Yee, Kim Jeongcho, Lee Hyung Mok, Kim Chunglee, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, Putten Maurice, H.P.M. van, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya, 樫山 和己, 八木 絢外, Pai Archana, 我妻 一博, 久徳 浩太郎

    日本物理学会講演概要集  2014.03  一般社団法人日本物理学会

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  • 26aBE-1 The current status of Large-scale Cryogenic Gravitational Wave Telescope (KAGRA) Project (8) Domestic conference

    Kawamura Seiji, Friedrich Daniel, Baiotti Luca, Chen Yanbei, Miao Haixing, Tobar M. E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, Zhu Zong-Hong, Dhurandhar S, Pai Archana, Mitra S, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, Marka Szabolcs, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Conte Roberto, Fiumara Vincenzo, Matta Vincenzo, Chiadini Francesco, Postiglione Fabio, Ni Wei-Tou, Zhai Xiang-hua, Xi Ping, Mei Hsien-Hao, Yoon Tai Hyun, Lee Hyung Won, Lee Hyung Mok, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, van Putten, Maurice H. P. M, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya

    Meeting abstracts of the Physical Society of Japan  2013.03  The Physical Society of Japan (JPS)

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  • 26aBE-1 The current status of Large-scale Cryogenic Gravitational Wave Telescope (KAGRA) Project (8) Domestic conference

    Kawamura Seiji, Friedrich Daniel, Baiotti Luca, Chen Yanbei, Miao Haixing, Tobar M. E, Blair D, Li Ju, Zhao Chunnong, Wen Linqing, Johnson Warren, Zhu Zong-Hong, Dhurandhar S, Pai Archana, Mitra S, Milyukov V, Baggio Lucio, Zhang Yang, Cao Junwei, Pan Sheau-Shi, Chen Sheng-Jui, Marka Szabolcs, Reid Stuart, Pinto Innocenzo, Galdi Vincenzo, Pierro Vincenzo, Castaldi Giuseppe, DeSalvo Riccardo, Croce Rocco P, Principe Maria, Conte Roberto, Fiumara Vincenzo, Matta Vincenzo, Chiadini Francesco, Postiglione Fabio, Ni Wei-Tou, Zhai Xiang-hua, Xi Ping, Mei Hsien-Hao, Yoon Tai Hyun, Lee Hyung Won, Lee Hyung Mok, Kim Jae Wan, Cha Yong-Ho, Lee Hyun Kyu, Lee Chang-Hwan, Kang Gungwon, Oh John J, Oh Sang Hoon, Park Myeong-Gu, Kim Sang Pyo, van Putten, Maurice H. P. M, Kyuman Cho, Xu Jun, Zheng Lihe, Wang Jingya

    Meeting abstracts of the Physical Society of Japan  2013.03  The Physical Society of Japan (JPS)

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  • 26pBE-3 Control for KAGRA using digital system (IV) Domestic conference

    Miyakawa O, Michimura Y, Miyoki S, Yamamoto T, Yuzurihara H, KAGRA Collaboration, Aso Y, Izumi K, Uchiyama T, Ohishi N, Kamiizumi M, Kanda N, Tanaka K, Hayama K

    Meeting Abstracts of the Physical Society of Japan  2013  The Physical Society of Japan

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  • 26pBE-3 Control for KAGRA using digital system (IV) Domestic conference

    Miyakawa O, Michimura Y, Miyoki S, Yamamoto T, Yuzurihara H, KAGRA Collaboration, Aso Y, Izumi K, Uchiyama T, Ohishi N, Kamiizumi M, Kanda N, Tanaka K, Hayama K

    Meeting Abstracts of the Physical Society of Japan  2013  The Physical Society of Japan

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  • 21pBL-7 重力波検出器の現状と将来計画(21pBL 宇宙線・宇宙物理領域シンポジウム:一般相対論の直接検証:ブラックホール・シャドーの直接撮像と重力波の検出,宇宙線・宇宙物理領域) Domestic conference

    神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集  2010 

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  • 21pBL-7 重力波検出器の現状と将来計画(21pBL 宇宙線・宇宙物理領域シンポジウム:一般相対論の直接検証:ブラックホール・シャドーの直接撮像と重力波の検出,宇宙線・宇宙物理領域) Domestic conference

    神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集  2010 

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  • 24pZW-2 干渉計型重力波検出器TAMA300開発の現状XX(干渉計開発)(重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 石崎 秀晴, 中川 憲保, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 辰巳 大輔, 安東 正樹, 三代木 伸二, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 高橋 竜太郎, 坪野 公夫, TAMA Conaboration, 和泉 究, 我妻 一博, 荒瀬 勇太, 若林 野花, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2008 

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  • 24pZW-2 干渉計型重力波検出器TAMA300開発の現状XX(干渉計開発)(重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 石崎 秀晴, 中川 憲保, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 辰巳 大輔, 安東 正樹, 三代木 伸二, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 高橋 竜太郎, 坪野 公夫, TAMA Conaboration, 和泉 究, 我妻 一博, 荒瀬 勇太, 若林 野花, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2008 

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  • 21pZH-2 干渉計型重力波検出器TAMA300開発の現状 XV : 低周波防振装置2(21pZH 重力波,宇宙線・宇宙物理領域) Domestic conference

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 高橋 竜太郎, 森脇 成典, 神田 履行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴, 新井 宏二, 辰巳 大輔, 和泉 究

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 28pSG-5 宇宙線の干渉計型重力波検出器に対する影響(28pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    山元 一広, 常定 芳基, 岡田 淳, 内山 隆, 三代木 伸二, 大橋 正健, 黒田 和明, 早河 秀章, 神田 展行, 辰巳 大輔

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 27pSG-6 干渉計型重力波検出器TAMA300開発の現状XIII : 干渉計開発(27pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 森脇 成典, 辰巳 大輔, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 高橋 竜太郎, 中川 憲保, 我妻 一博, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 高森 昭光

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 21pZH-5 干渉計型重力波検出器TAMA300開発の現状 XVIII : 干渉計開発(21pZH 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 辰巳 大輔, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 和泉 究, 高橋 竜太郎, 我妻 一博, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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    Presentation type:Oral presentation (general)  

  • 21pZH-2 干渉計型重力波検出器TAMA300開発の現状 XV : 低周波防振装置2(21pZH 重力波,宇宙線・宇宙物理領域) Domestic conference

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 高橋 竜太郎, 森脇 成典, 神田 履行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴, 新井 宏二, 辰巳 大輔, 和泉 究

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 28pSG-5 宇宙線の干渉計型重力波検出器に対する影響(28pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    山元 一広, 常定 芳基, 岡田 淳, 内山 隆, 三代木 伸二, 大橋 正健, 黒田 和明, 早河 秀章, 神田 展行, 辰巳 大輔

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 27pSG-6 干渉計型重力波検出器TAMA300開発の現状XIII : 干渉計開発(27pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 森脇 成典, 辰巳 大輔, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 高橋 竜太郎, 中川 憲保, 我妻 一博, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 高森 昭光

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 21pZH-5 干渉計型重力波検出器TAMA300開発の現状 XVIII : 干渉計開発(21pZH 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 麻生 洋一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 辰巳 大輔, 森脇 成典, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 和泉 究, 高橋 竜太郎, 我妻 一博, 荒瀬 勇太, 福嶋 美津広, 山崎 利孝, 石崎 秀晴

    一般社団法人 日本物理学会 日本物理学会講演概要集  2007 

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  • 20pSG-2 干渉計型重力波検出器TAMA300開発の現状VIII : 低周波防振装置(20pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 森脇 成典, 高橋 竜太郎, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 辰巳 大輔, 麻生 洋一, 新井 宏二, 中川 憲保, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-8 多変量クラスターを用いたTAMA300データのバースト重力波解析(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    本多 了太, 安東 正樹, 田越 秀行, 辰巳 大輔, 粟家 律親, 徳田 充, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-7 ALFフィルタを用いたTAMA300データのバースト重力波解析IV(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    阿久津 朋美, 安東 正樹, 神田 展行, 辰巳 大輔, 寺田 聡一, 三代木 伸二, 大橋 正健, TAMA Collaboration

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-3 干渉計型重力波検出器TAMA300開発の現状VI : 要素技術(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    佐藤 修一, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 新井 宏二, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正健, 黒田 和明, the TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-2 干渉計型重力波検出器TAMA300開発の現状V : 干渉計開発(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 佐藤 修一, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正健, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 20pSG-5 TAMA300データを用いたGCC統計の評価(20pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    石徹白 晃治, 姫本 宣朗, 神田 展行, 安東 正樹, 坪野 公夫

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 20pSG-2 干渉計型重力波検出器TAMA300開発の現状VIII : 低周波防振装置(20pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    我妻 一博, 高森 昭光, Bertolini A, DeSalvo R, 佐藤 修一, 阿久津 智忠, 常定 芳基, 長野 重夫, 安東 正樹, 三代木 伸二, 森脇 成典, 高橋 竜太郎, 神田 展行, 武者 満, 藤本 眞克, 川村 静児, 三尾 典克, 大橋 正健, 黒田 和明, 坪野 公夫, TAMA Collaboration, 荒瀬 勇太, 辰巳 大輔, 麻生 洋一, 新井 宏二, 中川 憲保, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-8 多変量クラスターを用いたTAMA300データのバースト重力波解析(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    本多 了太, 安東 正樹, 田越 秀行, 辰巳 大輔, 粟家 律親, 徳田 充, 神田 展行

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-7 ALFフィルタを用いたTAMA300データのバースト重力波解析IV(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    阿久津 朋美, 安東 正樹, 神田 展行, 辰巳 大輔, 寺田 聡一, 三代木 伸二, 大橋 正健, TAMA Collaboration

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-3 干渉計型重力波検出器TAMA300開発の現状VI : 要素技術(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    佐藤 修一, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 新井 宏二, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正健, 黒田 和明, the TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 27aTG-2 干渉計型重力波検出器TAMA300開発の現状V : 干渉計開発(27aTG 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 佐藤 修一, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正健, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 20pSG-5 TAMA300データを用いたGCC統計の評価(20pSG 重力波,宇宙線・宇宙物理領域) Domestic conference

    石徹白 晃治, 姫本 宣朗, 神田 展行, 安東 正樹, 坪野 公夫

    一般社団法人 日本物理学会 日本物理学会講演概要集  2006 

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  • 15aSF-6 干渉計型重力波検出器TAMA300開発の現状II : 干渉計開発(15aSF 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 佐藤 修一, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正雄, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-9 レーザー干渉計型重力波検出器TAMA300のパワーリサイクリングXVIII(変調・復調系雑音)(重力波,宇宙線・宇宙物理) Domestic conference

    佐藤 修一, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 新井 宏二, 大橋 正健, 黒田 和明, the TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-8 レーザー干渉計型重力波検出器TAMA300のパワーリサイクリングXVII(検出器改良)(重力波,宇宙線・宇宙物理) Domestic conference

    新井 宏二, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 佐藤 修一, 大橋 正健, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-3 TAMA300データを用いたバースト重力波解析IV(重力波,宇宙線・宇宙物理) Domestic conference

    安東 花樹, 三尾 典克, 森脇 成典, 三代木 伸二, 近藤 寿浩, 麻生 洋一, 阿久津 智忠, 長野 重夫, TAMA Collaboration, 高橋 竜太郎, 新井 宏二, 佐藤 修一, 辰巳 大輔, 神田 展行, 常定 芳基, 山崎 利孝, 福嶋 美津広

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-2 ALFフィルタを用いたTAMA300データのバースト重力波解析(重力波,宇宙線・宇宙物理) Domestic conference

    阿久津 朋美, 黒田 和明, 安東 正樹, 神田 展行, 辰巳 大輔, 寺田 聡一, 早河 秀章, 山元 一広, 三代木 伸二, 大橋 正健

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-10 レー-ザー干渉計型重力波検出器TAMA300のパワーリサイクリングXIX(信号取得・制御系)(重力波,宇宙線・宇宙物理) Domestic conference

    中川 憲保, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 新井 宏二, 大橋 正健, 黒田 和明, TAMA Collaboration, 佐藤 修一, 高橋 竜太郎, 阿久津 智忠, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 15aSF-7 干渉計型重力波検出器TAMA300開発の現状III : 変調系雑音(15aSF 重力波,宇宙線・宇宙物理領域) Domestic conference

    佐藤 修一, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 新井 宏二, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正雄, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-9 レーザー干渉計型重力波検出器TAMA300のパワーリサイクリングXVIII(変調・復調系雑音)(重力波,宇宙線・宇宙物理) Domestic conference

    佐藤 修一, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 新井 宏二, 大橋 正健, 黒田 和明, the TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-8 レーザー干渉計型重力波検出器TAMA300のパワーリサイクリングXVII(検出器改良)(重力波,宇宙線・宇宙物理) Domestic conference

    新井 宏二, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 佐藤 修一, 大橋 正健, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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  • 26pXH-3 TAMA300データを用いたバースト重力波解析IV(重力波,宇宙線・宇宙物理) Domestic conference

    安東 花樹, 三尾 典克, 森脇 成典, 三代木 伸二, 近藤 寿浩, 麻生 洋一, 阿久津 智忠, 長野 重夫, TAMA Collaboration, 高橋 竜太郎, 新井 宏二, 佐藤 修一, 辰巳 大輔, 神田 展行, 常定 芳基, 山崎 利孝, 福嶋 美津広

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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    Presentation type:Oral presentation (general)  

  • 26pXH-2 ALFフィルタを用いたTAMA300データのバースト重力波解析(重力波,宇宙線・宇宙物理) Domestic conference

    阿久津 朋美, 黒田 和明, 安東 正樹, 神田 展行, 辰巳 大輔, 寺田 聡一, 早河 秀章, 山元 一広, 三代木 伸二, 大橋 正健

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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    Presentation type:Oral presentation (general)  

  • 26pXH-10 レー-ザー干渉計型重力波検出器TAMA300のパワーリサイクリングXIX(信号取得・制御系)(重力波,宇宙線・宇宙物理) Domestic conference

    中川 憲保, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 武者 満, 神田 展行, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 新井 宏二, 大橋 正健, 黒田 和明, TAMA Collaboration, 佐藤 修一, 高橋 竜太郎, 阿久津 智忠, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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    Presentation type:Oral presentation (general)  

  • 15aSF-7 干渉計型重力波検出器TAMA300開発の現状III : 変調系雑音(15aSF 重力波,宇宙線・宇宙物理領域) Domestic conference

    佐藤 修一, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 新井 宏二, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正雄, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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    Presentation type:Oral presentation (general)  

  • 15aSF-6 干渉計型重力波検出器TAMA300開発の現状II : 干渉計開発(15aSF 重力波,宇宙線・宇宙物理領域) Domestic conference

    新井 宏二, 高森 昭光, 飯田 幸美, Bertolini A, DeSalvo R, 三代木 伸二, 長野 重夫, 安東 正樹, 森脇 成典, 神田 展行, 武者 満, 佐藤 修一, 三尾 典克, 川村 静児, 藤本 眞克, 坪野 公夫, 大橋 正雄, 黒田 和明, TAMA Collaboration, 高橋 竜太郎, 阿久津 智忠, 中川 憲保, 辰巳 大輔, 常定 芳基, 福嶋 美津広, 山崎 利孝

    一般社団法人 日本物理学会 日本物理学会講演概要集  2005 

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    Presentation type:Oral presentation (general)  

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Works

  • Study of vibration isolation system with ultra-long period X-pendulum for Gravitational Wave interferometer

    1994

  • Research of resonant gravitational wave antenna

    1993

  • Research of laser interferometer for resonant gravitational wave antenna

    1993

Grant-in-Aid for Scientific Research

  • 短時間ラプラス変換を応用したブラックホール準固有振動解析

    Grant-in-Aid for Scientific Research(C)  2025

  • 短時間ラプラス変換を応用したブラックホール準固有振動解析

    Grant-in-Aid for Scientific Research(C)  2024

  • DecipheringPhysics of Core-Collapse Supernovae via Gravitational-wave Astronomy

    Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area)  2017.06

  • Calibration Standard and High-Precision Data Analysis toward the Observational Era of Gravitational Waves

    Grant-in-Aid for Scientific Research(S)  2017.05

  • GPGPU advanced parallelization calculation for KAGRA data analysis

    Grant-in-Aid for Scientific Research(C)  2014.04

  • Research on Data Analysis of Gravitational Wave Searches Link up with Various Observations

    Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area)  2012.06

  • New development in astrophysics through multi messenger observation of gravitational wave sources

    Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area)  2012.06

  • Development of High-Speed Processing of Gravitational Wave Radiometry using GPGPU

    Grant-in-Aid for Scientific Research(C)  2011

  • Inspection of Laser-Axion Experiment PVLAS

    Grant-in-Aid for Young Scientists(A)  2008

  • 干渉計のデータ処理とイベント選別・相関解析

    Grant-in-Aid for Scientific Research on Priority Areas  2002

  • Education of Physics Experiment using Michelson Interferometer

    Grant-in-Aid for Scientific Research(C)  2001

  • Material Development for Understanding Optical Phenomena in Substances Using Polarization

    Grant-in-Aid for Scientific Research(C)  2000

  • Teaching materials development of optics using new materials and personal computers at elementary school and high school.

    Grant-in-Aid for Scientific Research(C)  1998

  • High Energy Cosmic Ray Background for Resonant-Mass Gravitational Wave Antenna

    Grant-in-Aid for Scientific Research(B)  1996

  • Gravitational Wave Astronomy using a Sensitive Laser Interferometer

    Grant-in-Aid for Creative Basic Research  1995

  • Development of a passive anti-vibration system in a frequency region of 1 Hz

    Grant-in-Aid for Scientific Research(A)  1995

  • ファブリ=ペロ-型レーザー干渉計を用いた微細構造定数の時間変化の測定開発

    奨励研究(A)  1994

  • Resonant Antenna for Monitoring Gravitational Wave Bursts in our Galaxy

    Grant-in-Aid for General Scientific Research (A)  1993

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Outline of education staff

  • Physics

Charge of on-campus class subject

  • 専門物理学実験A

    2024   Weekly class   Undergraduate

  • 物理実験学A

    2024   Weekly class   Undergraduate

  • 物理学特別研究2A

    2024   Intensive lecture   Graduate school

  • 物理学特別研究1A

    2024   Intensive lecture   Graduate school

  • 物理学特別演習2A

    2024   Intensive lecture   Graduate school

  • 物理学特別演習1A

    2024   Intensive lecture   Graduate school

  • 宇宙物理学

    2024   Weekly class   Graduate school

  • 物理学特別研究5A

    2024   Intensive lecture   Graduate school

  • 物理学特別研究4A

    2024   Intensive lecture   Graduate school

  • 物理学特別研究3A

    2024   Intensive lecture   Graduate school

  • 物理学特別演習5A

    2024   Intensive lecture   Graduate school

  • 物理学特別演習4A

    2024   Intensive lecture   Graduate school

  • 物理学特別演習3A

    2024   Intensive lecture   Graduate school

  • 宇宙物理学

    2019     Graduate school

  • 物理実験学

    2019     Undergraduate

  • 専門物理学実験

    2019     Undergraduate

  • 体験で知る科学と技術

    2019     Undergraduate

  • 計算科学

    2019     Graduate school

  • 物理実験学

    2018     Undergraduate

  • 専門物理学実験

    2018     Undergraduate

  • 計算科学

    2018     Graduate school

  • 基礎物理学I-E

    2018     Undergraduate

  • 体験で知る科学と技術

    2018     Undergraduate

  • 宇宙・高エネルギー物理学ゼミナール

    2018     Graduate school

  • 後期特別研究

    2018     Graduate school

  • 宇宙・高エネルギー物理学演習

    2018     Graduate school

  • 前期特別研究

    2018     Graduate school

  • 宇宙物理学

    2018     Graduate school

  • 専門物理学実験

    2017     Undergraduate

  • 物理実験学

    2017     Undergraduate

  • 体験で知る科学と技術

    2017     Undergraduate

  • 宇宙・高エネルギー物理学ゼミナール

    2017     Graduate school

  • 後期特別研究

    2017     Graduate school

  • 宇宙・高エネルギー物理学演習

    2017     Graduate school

  • 前期特別研究

    2017     Graduate school

  • 宇宙物理学

    2017     Graduate school

  • 重力波実験物理学

    2017     Graduate school

  • 実験で知る自然環境と人間

    2012     Undergraduate

  • 電磁気学とその演習

    2009     Undergraduate

  • 基礎物理学I

    2009     Undergraduate

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Original item・Special report (Education Activity)

  • 2019

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    Original item:「宇宙(天文)を学べる大学合同進学説明会」運営および参加

  • 2018

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    Original item:「宇宙(天文)を学べる大学合同進学説明会」運営および参加

Social Activities ⇒ Link to the list of Social Activities

  • 天文学者大集合 宇宙を学ぶ大学紹介イベント −第15回「“宇宙(天文)を学べる大学”合同進学説明会」−

    Role(s): Official expert, Planner, Logistic support

    Type: Lecture

    宇宙(天文)を学べる大学合同進学説明会実行委員会、大阪市立科学館  2022.06

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    Audience: High school students, University students, Teachers, Parents/Guardians, General public

    今年も関西を中心に全国各地の宇宙や天文を学べる大学から、天文学者・宇宙科学者である教員スタッフが合同進学説明会として集まります。昨年一昨年とオンラインで多数の方にご覧いただきました。今年は、オンラインに加えて、高校生・受験生に限定ですが大阪市立科学館の現地での対面も加えてハイブリッド形式で開催いたします。
    天文学者・宇宙科学者が集まって生の声が聞けるチャンスです。大学や研究室とはどういうところなのか、各大学の研究室にはどんな教員がいて具体的にどんな研究活動や教育活動をしているのか、研究室の雰囲気や出身学生の就職先なども含め、宇宙(天文)を学べる大学および研究室での活動を総合的に紹介します。また、ミニ天文講演会も開催いたします。以上はどなたでもオンライン(YouTube LIVE)での中継をご覧いただけます。

  • 天文学者大集合!宇宙を学ぶ大学紹介イベント −第14回「“宇宙(天文)を学べる大学”合同進学説明会」−

    Role(s): Guest, Host, Lecturer, Consultant, Planner, Logistic support

    Type: University open house, Cooperation business with The administrative, educational institutions, etc.

    宇宙(天文)を学べる大学合同進学説明会実行委員会、大阪市立科学館  天文学者大集合!宇宙を学ぶ大学紹介イベント −第14回「“宇宙(天文)を学べる大学”合同進学説明会」−  オンライン中継(参加者:大阪市立科学館、各大学)  2021.06

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    Audience: High school students, University students, Teachers, General public

    Number of participants:500(人)

  • 天文学者大集合!宇宙を学ぶ大学紹介イベント −第14回「“宇宙(天文)を学べる大学”合同進学説明会」−

    Role(s): Guest, Host, Planner, Logistic support

    Type: Lecture

    大阪市立科学館ほか  2021.06

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    Audience: High school students, University students, Teachers, Parents/Guardians, General public

  • 『超新星爆発と中性子星〜重力波で探る元素の起源〜』

    Role(s): Lecturer

    Type: Internet

    南部陽一郎物理学研究所オンライン市民講座  2021.03

  • 天文学者大集合!宇宙を学ぶ大学紹介イベント −第13回「“宇宙(天文)を学べる大学”合同進学説明会」−

    Role(s): Guest, Host, Planner, Logistic support

    Type: Lecture

    大阪市立科学館、各大学  2020.09

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    Audience: High school students, University students, Teachers, Parents/Guardians, General public, Civic organization

  • 天文学者大集合!宇宙を学ぶ大学紹介イベント −第12回「“宇宙(天文)を学べる大学”合同進学説明会」−

    Role(s): Guest, Host, Planner, Logistic support, Report author

    Type: Lecture

    大阪市立科学館  2019.06

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    Audience: High school students, University students, Teachers, Parents/Guardians, General public

  • 全国同時七夕講演会

    Role(s): Lecturer, Planner, Logistic support

    Type: Lecture

    大阪市立科学館  2013.07

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    Audience: General public

    Number of participants:197(人)

  • 全国同時七夕講演会

    Role(s): Lecturer, Planner, Logistic support

    Type: Lecture

    大阪市立科学館  2013.07

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    Audience: General public

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Foreigner acceptance

  • 2017

    foreigners accepted :3

Job title

  • Job title within the department

    Organization for Research Promotion 南部陽一郎物理学研究所 

    所長  2024.11

Other

  • Job Career

    2002.04 - Now

      More details

    Osaka City University Graduate School of Science Professor