Abstract
Original language | English |
---|---|
Pages (from-to) | 1 - 14 |
Number of pages | 14 |
Journal | Physical Review Letters |
Volume | 113 |
Issue number | 1 |
DOIs | |
Publication status | Published - 2014 |
Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver
}
In: Physical Review Letters, Vol. 113, No. 1, 2014, p. 1 - 14.
Research output: Contribution to journal › Article › Research › peer-review
TY - JOUR
T1 - Search for gravitational waves associated with gamma-ray bursts detected by the interplanetary network
AU - Aasi, Junaid
AU - Abbott, Benjamin P
AU - Abbott, Richard S
AU - Abbott, Thomas
AU - Abernathy, Matthew Robert
AU - Acernese, Fausto
AU - Ackley, Kendall
AU - Adams, Catherine Anne
AU - Adams, Thomas S
AU - Addesso, Paolo
AU - Adhikari, Rana X
AU - Affeldt, Christoph
AU - Agathos, Michalis
AU - Aggarwal, Nancy
AU - Aguiar, Odylio D
AU - Ajith, Parameswaran M
AU - Alemic, Almir
AU - Allen, Bruce
AU - Allocca, Annalisa
AU - Amariutei, Daniel
AU - Andersen, Mathis Baekbo
AU - Anderson, R A
AU - Anderson, Stuart B
AU - Anderson, Warren G
AU - Arai, Koji
AU - Araya, Melody C
AU - Arceneaux, Cody Christopher
AU - Areeda, Joseph S
AU - Ast, Stefan
AU - Aston, Stuart M
AU - Astone, Pia
AU - Aufmuth, Peter
AU - Augustus, H
AU - Aulbert, Carsten
AU - Aylott, Benjamin Edwin
AU - Babak, Stanislav
AU - Baker, Paul T
AU - Ballardin, G
AU - Ballmer, Stefan W
AU - Barayoga, Juan C
AU - Barbet, Mark
AU - Barish, Barry C
AU - Barker, David
AU - Barone, Fabrizio
AU - Barr, Bryan W
AU - Barsotti, Lisa
AU - Barsuglia, Matteo
AU - Barton, Mark A
AU - Bartos, Imre
AU - Bassiri, Riccardo
AU - Basti, A
AU - Batch, Jim C
AU - Bauchrowitz, Joran
AU - Bauer, Th S
AU - Baune, Christoph
AU - Bavigadda, Viswanath
AU - Behnke, Berit
AU - Bejger, Michal
AU - Beker, M G
AU - Belczynski, Chris
AU - Bell, Angus S
AU - Bell, C
AU - Bergmann, Gerald
AU - Bersanetti, Diego
AU - Bertolini, Alessandro
AU - Betzwieser, Joseph C
AU - Bilenko, Igor Antonovich
AU - Billingsley, GariLynn
AU - Birch, Jeremy
AU - Biscans, Sebastien
AU - Bitossi, Massimiliano
AU - Biwer, Christoph M
AU - Bizouard, Marie-Anne
AU - Black, Eric
AU - Blackburn, James Kent
AU - Blackburn, Lindy L
AU - Blair, David G
AU - Bloemen, Steven
AU - Bock, O
AU - Bodiya, Timothy Paul
AU - Boer, M
AU - Bogaert, Gilles
AU - Bogan, Christina
AU - Bond, Charlotte
AU - Bondu, Francois
AU - Bonelli, L
AU - Bonnand, Romain
AU - Bork, Rolf
AU - Born, Michael
AU - Boschi, Valerio
AU - Bose, Sukanta
AU - Bosi, Leone
AU - Bradaschia, Carlo
AU - Brady, Patrick R
AU - Braginsky, Vladimir Borisovich
AU - Branchesi, Marica
AU - Brau, James E
AU - Briant, T
AU - Bridges, D O
AU - Brillet, Alain
AU - Brinkmann, Marc
AU - Brisson, Violette
AU - Brooks, Aidan F
AU - Brown, Duncan Alexander
AU - Brown, Daniel D
AU - Bruckner, Frank
AU - Buchman, Saps
AU - Buikema, Aaron
AU - Bulik, Tomasz
AU - Bulten, Henk Jan
AU - Buonanno, Alessandra
AU - Burman, Ron
AU - Buskulic, Damir
AU - Buy, Christelle
AU - Cadonati, Laura
AU - Cagnoli, Gianpietro
AU - Calderon Bustillo, Juan
AU - Calloni, Enrico
AU - Camp, Jordan B
AU - Campsie, Paul
AU - Cannon, Kipp C
AU - Canuel, Benjamin
AU - Cao, J
AU - Capano, Collin D
AU - Carbognani, Franco
AU - Carbone, Ludovico
AU - Caride, Santiago
AU - Castaldi, Giuseppe
AU - Caudill, Sarah
AU - Cavaglia, Marco
AU - Cavalier, Fabien
AU - Cavalieri, Roberto
AU - Celerier, Charles
AU - Cella, Giancarlo
AU - Cepeda, Christian
AU - Cesarini, Elisabetta
AU - Chakraborty, Rijuparna
AU - Chalermsongsak, Tara
AU - Chamberlin, Sydney JoAnne
AU - Chao, Shiuh
AU - Charlton, Philip
AU - Chassande-Mottin, Eric
AU - Chen, Xu
AU - Chen, Yanbei
AU - Chincarini, Andrea
AU - Chiummo, Antonino
AU - Cho, Hee Suk
AU - Cho, Minkyoung
AU - Chow, Jong
AU - Christensen, Nelson
AU - Chu, Qi
AU - Chua, Sheon
AU - Chung, Shin Kee
AU - Ciani, Giacomo
AU - Clara, Filiberto
AU - Clark, Daniel E
AU - Clark, James A
AU - Clayton, Jessica H
AU - Cleva, Frederic
AU - Coccia, Eugenio
AU - Cohadon, Pierre-Francois
AU - Colla, Alberto
AU - Collette, Christophe Guy
AU - Colombini, Marco
AU - Cominsky, Lynn R
AU - Constancio Jr, Marcio
AU - Conte, A
AU - Cook, Douglas
AU - Corbitt, Thomas R
AU - Cornish, Neil
AU - Corsi, Alessandra
AU - Costa, Cesar A
AU - Coughlin, Michael William
AU - Coulon, Jean-Pierre
AU - Countryman, Stefan Trklja
AU - Couvares, Peter
AU - Coward, David M
AU - Cowart, Matthew
AU - Coyne, Dennis C
AU - Coyne, Robert
AU - Craig, Kieran
AU - Creighton, Jolien D E
AU - Croce, Rocco P
AU - Crowder, Sarah Gwynne
AU - Cumming, Alan
AU - Cunningham, Liam
AU - Cuoco, Elena
AU - Cutler, Curt J
AU - Dahl, Katrin
AU - Dal Canton, Tito
AU - Damjanic, M
AU - Danilishin, Stefan L
AU - D'Antonio, Sabrina
AU - Danzmann, K
AU - Dattilo, Vincenzino
AU - Daveloza, Hernan Pablo
AU - Davier, Michel
AU - Davies, Gareth Stephen
AU - Daw, Edward J
AU - Day, Richard Arthur
AU - Dayanga, Thilina
AU - DeBra, Daniel B
AU - Debreczeni, Gergely
AU - Degallaix, Jerome
AU - Deleglise, Samuel
AU - Del Pozzo, Walter
AU - Denker, Timo
AU - Dent, Thomas
AU - Dereli, Husne
AU - Dergachev, Vladimir
AU - De Rosa, Rosario D
AU - DeRosa, Ryan T
AU - DeSalvo, Riccardo
AU - Dhurandhar, Sanjeev Vishnu
AU - Diaz, Mario
AU - Dickson, J
AU - Di Fiore, Luciano
AU - Di Lieto, Alberto
AU - Di Palma, Irene
AU - Di Virgilio, Angela
AU - Dolique, Vincent
AU - Dominguez, E
AU - Donovan, Fred
AU - Dooley, Katherine L
AU - Doravari, Suresh
AU - Douglas, Rebecca
AU - Downes, Tom P
AU - Drago, Marco
AU - Drever, Ronald W P
AU - Driggers, Jenne
AU - Du, Zhengwei
AU - Ducrot, Marine
AU - Dwyer, Sheila E
AU - Eberle, Tobias
AU - Edo, Tega Boro
AU - Edwards, Mark
AU - Effler, Anamaria
AU - Eggenstein, Heinz-Bernd
AU - Ehrens, Phil
AU - Eichholz, Johannes
AU - Eikenberry, Stephen Scott
AU - Endroczi, Gabor
AU - Lasky, Paul Daniel
AU - Levin, Yuri
AU - Mandel, Ilya
AU - Premachandra, Sammanani Shakya
AU - Sammut, Letizia
AU - Smith, Robert James E
AU - Thrane, Eric
AU - Zhu, Xing J
AU - The LIGO Scientific Collaboration
AU - Virgo Collaboration
AU - the IPN Collaboration
PY - 2014
Y1 - 2014
N2 - We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005?2010 during LIGO?s fifth and sixth science runs and Virgo?s first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10-2M?c2 at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90 confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
AB - We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005?2010 during LIGO?s fifth and sixth science runs and Virgo?s first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10-2M?c2 at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90 confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
UR - http://journals.aps.org.ezproxy.lib.monash.edu.au/prl/pdf/10.1103/PhysRevLett.113.011102
U2 - 10.1103/PhysRevLett.113.011102
DO - 10.1103/PhysRevLett.113.011102
M3 - Article
SN - 0031-9007
VL - 113
SP - 1
EP - 14
JO - Physical Review Letters
JF - Physical Review Letters
IS - 1
ER -