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GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.

We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initia... Full description

Journal Title: Physical review letters June 17, 2016, Vol.116(24), p.241103
Main Author: Abbott, B P
Other Authors: 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 , Allen, B , Allocca, A , Altin, P A , Anderson, S B , Anderson, W G , Arai, K , Araya, M C , Arceneaux, C C , Areeda, J S , Arnaud, N , Arun, K G , Ascenzi, S , Ashton, G , Ast, M , Aston, S M , Astone, P , Aufmuth, P , Aulbert, C , Babak, S , Bacon, P , Bader, M K M , 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 , Bartos, I , Bassiri, R , Basti, A , Batch, J C , Baune, C , Bavigadda, V , Bazzan, M , Bejger, 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 , Birch, J , Birney, R , Birnholtz, O , Biscans, S , Bisht, A , Bitossi, M , Biwer, C , Bizouard, M A , Blackburn, J K , Blair, C D , Blair, D G , Blair, R M , Bloemen, S , Bock, O , Boer, M , Bogaert, G , Bogan, C , Bohe, A , Bond, C , 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 , Calderón Bustillo, J , Callister, T , Calloni, E , Camp, J B , Cannon, K C , Cao, J , Capano, C D , Capocasa, E , Carbognani, F , Caride, S , Casanueva Diaz, J , Casentini, C , Caudill, S , Cavaglià, M , Cavalier, F , Cavalieri, R , Cella, G , Cepeda, C B , Cerboni Baiardi, L , Cerretani, G , Cesarini, E , Chamberlin, S J , Chan, M , Chao, S , Charlton, P , Chassande-Mottin, E , Cheeseboro, B D , Chen, H Y , Chen, Y , Cheng, C , Chincarini, A , Chiummo, A , Cho, H S , Cho, M , Chow, J H , Christensen, N , Chu, Q , Chua, S , Chung, S , Ciani, G , Clara, F , Clark, J A , Cleva, F , Coccia, E , Cohadon, P-F , Colla, A , Collette, C G , Cominsky, L , Constancio, M , Conte, A , Conti, L , Cook, D , Corbitt, T R , Cornish, N , Corsi, A , Cortese, S , Costa, C A , Coughlin, M W , Coughlin, S B , Coulon, J-P , Countryman, S T , Couvares, P , Cowan, E E , Coward, D M , Cowart, M J , Coyne, D C , Coyne, R , Craig, K , Creighton, J D E , Cripe, J , Crowder, S G , Cumming, A , Cunningham, L , Cuoco, E , Dal Canton, T , Danilishin, S L , D'Antonio, S , Danzmann, K , Darman, N S , Dasgupta, A , Da Silva Costa, C F , Dattilo, V , Dave, I , Davier, M , Davies, G S , Daw, E J , Day, R , De, S , Debra, D , Debreczeni, G , Degallaix, J , De Laurentis, M , Deléglise, S , Del Pozzo, W , Denker, T , Dent, T , Dergachev, V , De Rosa, R , Derosa, R T , Desalvo, R , Devine, R C , Dhurandhar, S , Díaz, M C , Di Fiore, L , Di Giovanni, M , Di Girolamo, T , Di Lieto, A , Di Pace, S , Di Palma, I , Di Virgilio, A , Dolique, V , Donovan, F , Dooley, K L , Doravari, S , Douglas, R , Downes, T P , Drago, M , Drever, R W P , Driggers, J C , Ducrot, M , Dwyer, S E , Edo, T B
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1079-7114 ; DOI: 10.1103/PhysRevLett.116.241103
Link: http://search.proquest.com/docview/1801423278/?pq-origsite=primo
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title: GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
format: Article
creator:
  • 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
  • Allen, B
  • Allocca, A
  • Altin, P A
  • Anderson, S B
  • Anderson, W G
  • Arai, K
  • Araya, M C
  • Arceneaux, C C
  • Areeda, J S
  • Arnaud, N
  • Arun, K G
  • Ascenzi, S
  • Ashton, G
  • Ast, M
  • Aston, S M
  • Astone, P
  • Aufmuth, P
  • Aulbert, C
  • Babak, S
  • Bacon, P
  • Bader, M K M
  • 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
  • Bartos, I
  • Bassiri, R
  • Basti, A
  • Batch, J C
  • Baune, C
  • Bavigadda, V
  • Bazzan, M
  • Bejger, 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
  • Birch, J
  • Birney, R
  • Birnholtz, O
  • Biscans, S
  • Bisht, A
  • Bitossi, M
  • Biwer, C
  • Bizouard, M A
  • Blackburn, J K
  • Blair, C D
  • Blair, D G
  • Blair, R M
  • Bloemen, S
  • Bock, O
  • Boer, M
  • Bogaert, G
  • Bogan, C
  • Bohe, A
  • Bond, C
  • 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
  • Calderón Bustillo, J
  • Callister, T
  • Calloni, E
  • Camp, J B
  • Cannon, K C
  • Cao, J
  • Capano, C D
  • Capocasa, E
  • Carbognani, F
  • Caride, S
  • Casanueva Diaz, J
  • Casentini, C
  • Caudill, S
  • Cavaglià, M
  • Cavalier, F
  • Cavalieri, R
  • Cella, G
  • Cepeda, C B
  • Cerboni Baiardi, L
  • Cerretani, G
  • Cesarini, E
  • Chamberlin, S J
  • Chan, M
  • Chao, S
  • Charlton, P
  • Chassande-Mottin, E
  • Cheeseboro, B D
  • Chen, H Y
  • Chen, Y
  • Cheng, C
  • Chincarini, A
  • Chiummo, A
  • Cho, H S
  • Cho, M
  • Chow, J H
  • Christensen, N
  • Chu, Q
  • Chua, S
  • Chung, S
  • Ciani, G
  • Clara, F
  • Clark, J A
  • Cleva, F
  • Coccia, E
  • Cohadon, P-F
  • Colla, A
  • Collette, C G
  • Cominsky, L
  • Constancio, M
  • Conte, A
  • Conti, L
  • Cook, D
  • Corbitt, T R
  • Cornish, N
  • Corsi, A
  • Cortese, S
  • Costa, C A
  • Coughlin, M W
  • Coughlin, S B
  • Coulon, J-P
  • Countryman, S T
  • Couvares, P
  • Cowan, E E
  • Coward, D M
  • Cowart, M J
  • Coyne, D C
  • Coyne, R
  • Craig, K
  • Creighton, J D E
  • Cripe, J
  • Crowder, S G
  • Cumming, A
  • Cunningham, L
  • Cuoco, E
  • Dal Canton, T
  • Danilishin, S L
  • D'Antonio, S
  • Danzmann, K
  • Darman, N S
  • Dasgupta, A
  • Da Silva Costa, C F
  • Dattilo, V
  • Dave, I
  • Davier, M
  • Davies, G S
  • Daw, E J
  • Day, R
  • De, S
  • Debra, D
  • Debreczeni, G
  • Degallaix, J
  • De Laurentis, M
  • Deléglise, S
  • Del Pozzo, W
  • Denker, T
  • Dent, T
  • Dergachev, V
  • De Rosa, R
  • Derosa, R T
  • Desalvo, R
  • Devine, R C
  • Dhurandhar, S
  • Díaz, M C
  • Di Fiore, L
  • Di Giovanni, M
  • Di Girolamo, T
  • Di Lieto, A
  • Di Pace, S
  • Di Palma, I
  • Di Virgilio, A
  • Dolique, V
  • Donovan, F
  • Dooley, K L
  • Doravari, S
  • Douglas, R
  • Downes, T P
  • Drago, M
  • Drever, R W P
  • Driggers, J C
  • Ducrot, M
  • Dwyer, S E
  • Edo, T B
subjects:
  • General Relativity And Quantum Cosmology
  • Astrophysics - High Energy Astrophysical Phenomena
ispartof: Physical review letters, June 17, 2016, Vol.116(24), p.241103
description: We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5 $\sigma$. The signal persisted in the LIGO frequency band for approximately 1 s, increasing in frequency and amplitude over about 55 cycles from 35 to 450 Hz, and reached a peak gravitational strain of $3.4_{-0.9}^{+0.7} \times 10^{-22}$. The inferred source-frame initial black hole masses are $14.2_{-3.7}^{+8.3} M_{\odot}$ and $7.5_{-2.3}^{+2.3} M_{\odot}$ and the final black hole mass is $20.8_{-1.7}^{+6.1} M_{\odot}$. We find that at least one of the component black holes has spin greater than 0.2. This source is located at a luminosity distance of $440_{-190}^{+180}$ Mpc corresponding to a redshift $0.09_{-0.04}^{+0.03}$. All uncertainties define a 90 % credible interval. This second gravitational-wave observation provides improved constraints on stellar populations and on deviations from general relativity. Comment: 14 pages, 5 figures
language: eng
source:
identifier: E-ISSN: 1079-7114 ; DOI: 10.1103/PhysRevLett.116.241103
fulltext: no_fulltext
issn:
  • 10797114
  • 1079-7114
url: Link


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titleGW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
creatorAbbott, 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 ; Allen, B ; Allocca, A ; Altin, P A ; Anderson, S B ; Anderson, W G ; Arai, K ; Araya, M C ; Arceneaux, C C ; Areeda, J S ; Arnaud, N ; Arun, K G ; Ascenzi, S ; Ashton, G ; Ast, M ; Aston, S M ; Astone, P ; Aufmuth, P ; Aulbert, C ; Babak, S ; Bacon, P ; Bader, M K M ; 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 ; Bartos, I ; Bassiri, R ; Basti, A ; Batch, J C ; Baune, C ; Bavigadda, V ; Bazzan, M ; Bejger, 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 ; Birch, J ; Birney, R ; Birnholtz, O ; Biscans, S ; Bisht, A ; Bitossi, M ; Biwer, C ; Bizouard, M A ; Blackburn, J K ; Blair, C D ; Blair, D G ; Blair, R M ; Bloemen, S ; Bock, O ; Boer, M ; Bogaert, G ; Bogan, C ; Bohe, A ; Bond, C ; 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 ; Calderón Bustillo, J ; Callister, T ; Calloni, E ; Camp, J B ; Cannon, K C ; Cao, J ; Capano, C D ; Capocasa, E ; Carbognani, F ; Caride, S ; Casanueva Diaz, J ; Casentini, C ; Caudill, S ; Cavaglià, M ; Cavalier, F ; Cavalieri, R ; Cella, G ; Cepeda, C B ; Cerboni Baiardi, L ; Cerretani, G ; Cesarini, E ; Chamberlin, S J ; Chan, M ; Chao, S ; Charlton, P ; Chassande-Mottin, E ; Cheeseboro, B D ; Chen, H Y ; Chen, Y ; Cheng, C ; Chincarini, A ; Chiummo, A ; Cho, H S ; Cho, M ; Chow, J H ; Christensen, N ; Chu, Q ; Chua, S ; Chung, S ; Ciani, G ; Clara, F ; Clark, J A ; Cleva, F ; Coccia, E ; Cohadon, P-F ; Colla, A ; Collette, C G ; Cominsky, L ; Constancio, M ; Conte, A ; Conti, L ; Cook, D ; Corbitt, T R ; Cornish, N ; Corsi, A ; Cortese, S ; Costa, C A ; Coughlin, M W ; Coughlin, S B ; Coulon, J-P ; Countryman, S T ; Couvares, P ; Cowan, E E ; Coward, D M ; Cowart, M J ; Coyne, D C ; Coyne, R ; Craig, K ; Creighton, J D E ; Cripe, J ; Crowder, S G ; Cumming, A ; Cunningham, L ; Cuoco, E ; Dal Canton, T ; Danilishin, S L ; D'Antonio, S ; Danzmann, K ; Darman, N S ; Dasgupta, A ; Da Silva Costa, C F ; Dattilo, V ; Dave, I ; Davier, M ; Davies, G S ; Daw, E J ; Day, R ; De, S ; Debra, D ; Debreczeni, G ; Degallaix, J ; De Laurentis, M ; Deléglise, S ; Del Pozzo, W ; Denker, T ; Dent, T ; Dergachev, V ; De Rosa, R ; Derosa, R T ; Desalvo, R ; Devine, R C ; Dhurandhar, S ; Díaz, M C ; Di Fiore, L ; Di Giovanni, M ; Di Girolamo, T ; Di Lieto, A ; Di Pace, S ; Di Palma, I ; Di Virgilio, A ; Dolique, V ; Donovan, F ; Dooley, K L ; Doravari, S ; Douglas, R ; Downes, T P ; Drago, M ; Drever, R W P ; Driggers, J C ; Ducrot, M ; Dwyer, S E ; Edo, T B
ispartofPhysical review letters, June 17, 2016, Vol.116(24), p.241103
identifierE-ISSN: 1079-7114 ; DOI: 10.1103/PhysRevLett.116.241103
languageeng
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subjectGeneral Relativity And Quantum Cosmology ; Astrophysics - High Energy Astrophysical Phenomena;
descriptionWe report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5 $\sigma$. The signal persisted in the LIGO frequency band for approximately 1 s, increasing in frequency and amplitude over about 55 cycles from 35 to 450 Hz, and reached a peak gravitational strain of $3.4_{-0.9}^{+0.7} \times 10^{-22}$. The inferred source-frame initial black hole masses are $14.2_{-3.7}^{+8.3} M_{\odot}$ and $7.5_{-2.3}^{+2.3} M_{\odot}$ and the final black hole mass is $20.8_{-1.7}^{+6.1} M_{\odot}$. We find that at least one of the component black holes has spin greater than 0.2. This source is located at a luminosity distance of $440_{-190}^{+180}$ Mpc corresponding to a redshift $0.09_{-0.04}^{+0.03}$. All uncertainties define a 90 % credible interval. This second gravitational-wave observation provides improved constraints on stellar populations and on deviations from general relativity. Comment: 14 pages, 5 figures
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30Ascenzi, S
31Ashton, G
32Ast, M
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34Astone, P
35Aufmuth, P
36Aulbert, C
37Babak, S
38Bacon, P
39Bader, M K M
40Baker, P T
41Baldaccini, F
42Ballardin, G
43Ballmer, S W
44Barayoga, J C
45Barclay, S E
46Barish, B C
47Barker, D
48Barone, F
49Barr, B
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52Barta, D
53Bartlett, J
54Bartos, I
55Bassiri, R
56Basti, A
57Batch, J C
58Baune, C
59Bavigadda, V
60Bazzan, M
61Bejger, M
62Bell, A S
63Berger, B K
64Bergmann, G
65Berry, C P L
66Bersanetti, D
67Bertolini, A
68Betzwieser, J
69Bhagwat, S
70Bhandare, R
71Bilenko, I A
72Billingsley, G
73Birch, J
74Birney, R
75Birnholtz, O
76Biscans, S
77Bisht, A
78Bitossi, M
79Biwer, C
80Bizouard, M A
81Blackburn, J K
82Blair, C D
83Blair, D G
84Blair, R M
85Bloemen, S
86Bock, O
87Boer, M
88Bogaert, G
89Bogan, C
90Bohe, A
91Bond, C
92Bondu, F
93Bonnand, R
94Boom, B A
95Bork, R
96Boschi, V
97Bose, S
98Bouffanais, Y
99Bozzi, A
100...
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titleGW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
authorAbbott, 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 ; Allen, B ; Allocca, A ; Altin, P A ; Anderson, S B ; Anderson,...
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15Aguiar, O D
16Aiello, L
17Ain, A
18Ajith, P
19Allen, B
20Allocca, A
21Altin, P A
22Anderson, S B
23Anderson, W G
24Arai, K
25Araya, M C
26Arceneaux, C C
27Areeda, J S
28Arnaud, N
29Arun, K G
30Ascenzi, S
31Ashton, G
32Ast, M
33Aston, S M
34Astone, P
35Aufmuth, P
36Aulbert, C
37Babak, S
38Bacon, P
39Bader, M K M
40Baker, P T
41Baldaccini, F
42Ballardin, G
43Ballmer, S W
44Barayoga, J C
45Barclay, S E
46Barish, B C
47Barker, D
48Barone, F
49Barr, B
50Barsotti, L
51Barsuglia, M
52Barta, D
53Bartlett, J
54Bartos, I
55Bassiri, R
56Basti, A
57Batch, J C
58Baune, C
59Bavigadda, V
60Bazzan, M
61Bejger, M
62Bell, A S
63Berger, B K
64Bergmann, G
65Berry, C P L
66Bersanetti, D
67Bertolini, A
68Betzwieser, J
69Bhagwat, S
70Bhandare, R
71Bilenko, I A
72Billingsley, G
73Birch, J
74Birney, R
75Birnholtz, O
76Biscans, S
77Bisht, A
78Bitossi, M
79Biwer, C
80Bizouard, M A
81Blackburn, J K
82Blair, C D
83Blair, D G
84Blair, R M
85Bloemen, S
86Bock, O
87Boer, M
88Bogaert, G
89Bogan, C
90Bohe, A
91Bond, C
92Bondu, F
93Bonnand, R
94Boom, B A
95Bork, R
96Boschi, V
97Bose, S
98Bouffanais, Y
99Bozzi, A
100...
jtitlePhysical review letters
toplevelpeer_reviewed
delivery
delcategoryRemote Search Resource
fulltextno_fulltext
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1Abernathy
2Acernese
3Ackley
4Adams
5Addesso
6Adhikari
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8Affeldt
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10Agatsuma
11Aggarwal
12Aguiar
13Aiello
14Ain
15Ajith
16Allen
17Allocca
18Altin
19Anderson
20Arai
21Araya
22Arceneaux
23Areeda
24Arnaud
25Arun
26Ascenzi
27Ashton
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29Aston
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61Berry
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64Betzwieser
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66Bhandare
67Bilenko
68Billingsley
69Birch
70Birney
71Birnholtz
72Biscans
73Bisht
74Bitossi
75Biwer
76Bizouard
77Blackburn
78Blair
79Bloemen
80Bock
81Boer
82Bogaert
83Bogan
84Bohe
85Bond
86Bondu
87Bonnand
88Boom
89Bork
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91Bose
92Bouffanais
93Bozzi
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97Branchesi
98Brau
99Briant
100...
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0Abbott, B P
1Abbott, R
2Abbott, T D
3Abernathy, M R
4Acernese, F
5Ackley, K
6Adams, C
7Adams, T
8Addesso, P
9Adhikari, R X
10Adya, V B
11Affeldt, C
12Agathos, M
13Agatsuma, K
14Aggarwal, N
15Aguiar, O D
16Aiello, L
17Ain, A
18Ajith, P
19Allen, B
20Allocca, A
21Altin, P A
22Anderson, S B
23Anderson, W G
24Arai, K
25Araya, M C
26Arceneaux, C C
27Areeda, J S
28Arnaud, N
29Arun, K G
30Ascenzi, S
31Ashton, G
32Ast, M
33Aston, S M
34Astone, P
35Aufmuth, P
36Aulbert, C
37Babak, S
38Bacon, P
39Bader, M K M
40Baker, P T
41Baldaccini, F
42Ballardin, G
43Ballmer, S W
44Barayoga, J C
45Barclay, S E
46Barish, B C
47Barker, D
48Barone, F
49Barr, B
50Barsotti, L
51Barsuglia, M
52Barta, D
53Bartlett, J
54Bartos, I
55Bassiri, R
56Basti, A
57Batch, J C
58Baune, C
59Bavigadda, V
60Bazzan, M
61Bejger, M
62Bell, A S
63Berger, B K
64Bergmann, G
65Berry, C P L
66Bersanetti, D
67Bertolini, A
68Betzwieser, J
69Bhagwat, S
70Bhandare, R
71Bilenko, I A
72Billingsley, G
73Birch, J
74Birney, R
75Birnholtz, O
76Biscans, S
77Bisht, A
78Bitossi, M
79Biwer, C
80Bizouard, M A
81Blackburn, J K
82Blair, C D
83Blair, D G
84Blair, R M
85Bloemen, S
86Bock, O
87Boer, M
88Bogaert, G
89Bogan, C
90Bohe, A
91Bond, C
92Bondu, F
93Bonnand, R
94Boom, B A
95Bork, R
96Boschi, V
97Bose, S
98Bouffanais, Y
99Bozzi, A
100...
atitleGW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
jtitlePhysical review letters
risdate20160617
volume116
issue24
spage241103
epage241103
pages241103
eissn1079-7114
formatjournal
genrearticle
ristypeJOUR
doi10.1103/PhysRevLett.116.241103
urlhttp://search.proquest.com/docview/1801423278/
orcidid0000-0001-6487-5197
issn00319007
date2016-06-17