GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

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.L. Danilishin; J. Hennig; S. Hild; J. Steinlechner; S. Steinlechner; J.F.J. Van den Brand

doi:10.1103/PhysRevLett.119.141101

GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

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. AjithB. 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.L. Danilishin, J. Hennig, S. Hild, J. Steinlechner, S. Steinlechner, J.F.J. Van den Brand

Research output: Contribution to journal › Article › Academic › peer-review

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Abstract

On August 14, 2017 at 10:30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of less than or similar to 1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5(-3.0)(+5.7)M(circle dot) and 25.3(-4.2)(+2.8) M-circle dot (at the 90% credible level). The luminosity distance of the source is 540(-210)(+130) Mpc, corresponding to a redshift of z = 0.11(-0.04)(+0.03). A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg(2) using only the two LIGO detectors to 60 deg(2) using all three detectors. For the first time, we can test the nature of gravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.

Original language	English
Article number	141101
Number of pages	16
Journal	Physical Review Letters
Volume	119
Issue number	14
DOIs	https://doi.org/10.1103/PhysRevLett.119.141101
Publication status	Published - 6 Oct 2017
Externally published	Yes

Keywords

ADVANCED LIGO
RADIATION
CHOICE
TOOL

Access to Document

10.1103/PhysRevLett.119.141101

Cite this

Abbott, B. P., Abbott, R., Abbott, T. D., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Afrough, M., Agarwal, B., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., ... Van den Brand, J. F. J. (2017). GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence. Physical Review Letters, 119(14), [141101]. https://doi.org/10.1103/PhysRevLett.119.141101

@article{17dc0e22a4f547dba89daa77706ebcc0,

title = "GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence",

abstract = "On August 14, 2017 at 10:30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of less than or similar to 1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5(-3.0)(+5.7)M(circle dot) and 25.3(-4.2)(+2.8) M-circle dot (at the 90% credible level). The luminosity distance of the source is 540(-210)(+130) Mpc, corresponding to a redshift of z = 0.11(-0.04)(+0.03). A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg(2) using only the two LIGO detectors to 60 deg(2) using all three detectors. For the first time, we can test the nature of gravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.",

keywords = "ADVANCED LIGO, RADIATION, CHOICE, TOOL",

author = "B.P. Abbott and R. Abbott and T.D. Abbott and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and R.X. Adhikari and V.B. Adya and C. Affeldt and M. Afrough and B. Agarwal and M. Agathos and K. Agatsuma and N. Aggarwal and O.D. Aguiar and L. Aiello and A. Ain and P. Ajith and B. Allen and G. Allen and A. Allocca and P.A. Altin and A. Amato and A. Ananyeva and S.B. Anderson and W.G. Anderson and S.V. Angelova and S. Antier and S. Appert and K. Arai and M.C. Araya and J.S. Areeda and N. Arnaud and K.G. Arun and S. Ascenzi and G. Ashton and M. Ast and S.M. Aston and P. Astone and D.V. Atallah and P. Aufmuth and C. Aulbert and K. AultONeal and C. Austin and A. Avila-Alvarez and S. Babak and P. Bacon and M.K.M. Bader and S.L. Danilishin and J. Hennig and S. Hild and J. Steinlechner and S. Steinlechner and {Van den Brand}, J.F.J.",

year = "2017",

month = oct,

day = "6",

doi = "10.1103/PhysRevLett.119.141101",

language = "English",

volume = "119",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "14",

}

Abbott, BP, Abbott, R, Abbott, TD, Acernese, F, Ackley, K, Adams, C, Adams, T, Addesso, P, Adhikari, RX, Adya, VB, Affeldt, C, Afrough, M, Agarwal, B, Agathos, M, Agatsuma, K, Aggarwal, N, Aguiar, OD, Aiello, L, Ain, A, Ajith, P, Allen, B, Allen, G, Allocca, A, Altin, PA, Amato, A, Ananyeva, A, Anderson, SB, Anderson, WG, Angelova, SV, Antier, S, Appert, S, Arai, K, Araya, MC, Areeda, JS, Arnaud, N, Arun, KG, Ascenzi, S, Ashton, G, Ast, M, Aston, SM, Astone, P, Atallah, DV, Aufmuth, P, Aulbert, C, AultONeal, K, Austin, C, Avila-Alvarez, A, Babak, S, Bacon, P, Bader, MKM, Danilishin, SL , Hennig, J , Hild, S , Steinlechner, J , Steinlechner, S & Van den Brand, JFJ 2017, 'GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence', Physical Review Letters, vol. 119, no. 14, 141101. https://doi.org/10.1103/PhysRevLett.119.141101

TY - JOUR

T1 - GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

AU - Abbott, B.P.

AU - Abbott, R.

AU - Abbott, T.D.

AU - Acernese, F.

AU - Ackley, K.

AU - Adams, C.

AU - Adams, T.

AU - Addesso, P.

AU - Adhikari, R.X.

AU - Adya, V.B.

AU - Affeldt, C.

AU - Afrough, M.

AU - Agarwal, B.

AU - Agathos, M.

AU - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O.D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Allen, B.

AU - Allen, G.

AU - Allocca, A.

AU - Altin, P.A.

AU - Amato, A.

AU - Ananyeva, A.

AU - Anderson, S.B.

AU - Anderson, W.G.

AU - Angelova, S.V.

AU - Antier, S.

AU - Appert, S.

AU - Arai, K.

AU - Araya, M.C.

AU - Areeda, J.S.

AU - Arnaud, N.

AU - Arun, K.G.

AU - Ascenzi, S.

AU - Ashton, G.

AU - Ast, M.

AU - Aston, S.M.

AU - Astone, P.

AU - Atallah, D.V.

AU - Aufmuth, P.

AU - Aulbert, C.

AU - AultONeal, K.

AU - Austin, C.

AU - Avila-Alvarez, A.

AU - Babak, S.

AU - Bacon, P.

AU - Bader, M.K.M.

AU - Danilishin, S.L.

AU - Hennig, J.

AU - Hild, S.

AU - Steinlechner, J.

AU - Steinlechner, S.

AU - Van den Brand, J.F.J.

PY - 2017/10/6

Y1 - 2017/10/6

N2 - On August 14, 2017 at 10:30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of less than or similar to 1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5(-3.0)(+5.7)M(circle dot) and 25.3(-4.2)(+2.8) M-circle dot (at the 90% credible level). The luminosity distance of the source is 540(-210)(+130) Mpc, corresponding to a redshift of z = 0.11(-0.04)(+0.03). A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg(2) using only the two LIGO detectors to 60 deg(2) using all three detectors. For the first time, we can test the nature of gravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.

AB - On August 14, 2017 at 10:30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of less than or similar to 1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5(-3.0)(+5.7)M(circle dot) and 25.3(-4.2)(+2.8) M-circle dot (at the 90% credible level). The luminosity distance of the source is 540(-210)(+130) Mpc, corresponding to a redshift of z = 0.11(-0.04)(+0.03). A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg(2) using only the two LIGO detectors to 60 deg(2) using all three detectors. For the first time, we can test the nature of gravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.

KW - ADVANCED LIGO

KW - RADIATION

KW - CHOICE

KW - TOOL

U2 - 10.1103/PhysRevLett.119.141101

DO - 10.1103/PhysRevLett.119.141101

M3 - Article

VL - 119

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 14

M1 - 141101

ER -