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

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • The LIGO Scientific Collaboration
  • Virgo Collaboration
  • the KAGRA Collaboration
  • K. Danzmann
  • M. Heurs
  • A. Hreibi
  • J. Lehmann
  • H. Lück
  • H. Vahlbruch
  • D. Wilken
  • B. Willke
  • D. S. Wu
  • C. Affeldt
  • F. Bergamin
  • A. Bisht
  • N. Bode
  • P. Booker
  • M. Brinkmann
  • N. Gohlke
  • A. Heidt
  • J. Heinze
  • S. Hochheim
  • W. Kastaun
  • R. Kirchhoff
  • P. Koch
  • N. Koper
  • V. Kringel
  • N. V. Krishnendu
  • G. Kuehn
  • S. Leavey
  • J. Liu
  • J. D. Lough
  • M. Matiushechkina
  • M. Mehmet
  • F. Meylahn
  • Nikhil Mukund
  • S. L. Nadji
  • M. Nery
  • F. Ohme
  • M. Schneewind
  • B. W. Schulte
  • B. F. Schutz
  • J. Venneberg
  • J. von Wrangel
  • M. Weinert
  • F. Wellmann
  • P. Weßels
  • W. Winkler
  • J. Woehler
  • Jonas Junker

Organisationseinheiten

Externe Organisationen

  • Australian National University
  • Maastricht University
  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • Universität Hamburg
  • Cardiff University
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer041039
FachzeitschriftPhysical Review X
Jahrgang13
Ausgabenummer4
PublikationsstatusVeröffentlicht - 4 Dez. 2023

Abstract

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 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 \(p_\mathrm{astro} > 0.5\). 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 \(p_\mathrm{astro} > 0.5\) 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 \(p_\mathrm{astro} > 0.5\) 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.

ASJC Scopus Sachgebiete

Zitieren

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run. / The LIGO Scientific Collaboration; Virgo Collaboration; the KAGRA Collaboration et al.
in: Physical Review X, Jahrgang 13, Nr. 4, 041039, 04.12.2023.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

The LIGO Scientific Collaboration, Virgo Collaboration, the KAGRA Collaboration, Danzmann, K, Heurs, M, Hreibi, A, Lehmann, J, Lück, H, Vahlbruch, H, Wilken, D, Willke, B, Wu, DS, Affeldt, C, Bergamin, F, Bisht, A, Bode, N, Booker, P, Brinkmann, M, Gohlke, N, Heidt, A, Heinze, J, Hochheim, S, Kastaun, W, Kirchhoff, R, Koch, P, Koper, N, Kringel, V, Krishnendu, NV, Kuehn, G, Leavey, S, Liu, J, Lough, JD, Matiushechkina, M, Mehmet, M, Meylahn, F, Mukund, N, Nadji, SL, Nery, M, Ohme, F, Schneewind, M, Schulte, BW, Schutz, BF, Venneberg, J, von Wrangel, J, Weinert, M, Wellmann, F, Weßels, P, Winkler, W, Woehler, J & Junker, J 2023, 'GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run', Physical Review X, Jg. 13, Nr. 4, 041039. https://doi.org/10.1103/PhysRevX.13.041039
The LIGO Scientific Collaboration, Virgo Collaboration, the KAGRA Collaboration, Danzmann, K., Heurs, M., Hreibi, A., Lehmann, J., Lück, H., Vahlbruch, H., Wilken, D., Willke, B., Wu, D. S., Affeldt, C., Bergamin, F., Bisht, A., Bode, N., Booker, P., Brinkmann, M., Gohlke, N., ... Junker, J. (2023). GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run. Physical Review X, 13(4), Artikel 041039. https://doi.org/10.1103/PhysRevX.13.041039
The LIGO Scientific Collaboration, Virgo Collaboration, the KAGRA Collaboration, Danzmann K, Heurs M, Hreibi A et al. GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run. Physical Review X. 2023 Dez 4;13(4):041039. doi: 10.1103/PhysRevX.13.041039
The LIGO Scientific Collaboration ; Virgo Collaboration ; the KAGRA Collaboration et al. / GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run. in: Physical Review X. 2023 ; Jahrgang 13, Nr. 4.
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@article{37769297372c4d71b4364ee05be8a5a7,
title = "GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run",
abstract = " 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 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 \(p_\mathrm{astro} > 0.5\). 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 \(p_\mathrm{astro} > 0.5\) 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 \(p_\mathrm{astro} > 0.5\) 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. ",
keywords = "gr-qc, astro-ph.HE",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and {the KAGRA Collaboration} and R. Abbott and Adya, {V. B.} and S. Bose and J. Brandt and Brown, {D. D.} and C. Chatterjee and X. Chen and Y.-B. Chen and Y.-R. Chen and H. Cheng and Choudhary, {R. K.} and S. Danilishin and K. Danzmann and H.-K. Guo and H. Hansen and J. Hennig and M. Heurs and A. Hreibi and H{\"u}bner, {M. T.} and K. Isleif and Lang, {R. N.} and Lee, {H. K.} and Lee, {H. M.} and Lee, {H. M.} and J. Lee and J. Lehmann and J. Li and X. Li and H. L{\"u}ck and A. More and T. Nguyen and L. Richardson and Rose, {C. A.} and S. Roy and Sanders, {J. R.} and P. Schmidt and S. Schmidt and L. Sun and H. Vahlbruch and D. Wilken and B. Willke and Wu, {D. S.} and H. Wu and Kohei Yamamoto and H. Zhang and L. Zhang and Y. Zhang and Y. Zheng and Z. Zhou and Zhu, {X. J.} and C. Affeldt and F. Bergamin and A. Bisht and N. Bode and P. Booker and M. Brinkmann and N. Gohlke and A. Heidt and J. Heinze and S. Hochheim and W. Kastaun and R. Kirchhoff and P. Koch and N. Koper and V. Kringel and Krishnendu, {N. V.} and G. Kuehn and S. Leavey and J. Liu and Lough, {J. D.} and M. Matiushechkina and M. Mehmet and F. Meylahn and Nikhil Mukund and Nadji, {S. L.} and M. Nery and F. Ohme and M. Schneewind and Schulte, {B. W.} and Schutz, {B. F.} and J. Venneberg and {von Wrangel}, J. and M. Weinert and F. Wellmann and P. We{\ss}els and W. Winkler and J. Woehler and Jonas Junker",
year = "2023",
month = dec,
day = "4",
doi = "10.1103/PhysRevX.13.041039",
language = "English",
volume = "13",
journal = "Physical Review X",
issn = "2160-3308",
publisher = "American Physical Society",
number = "4",

}

Download

TY - JOUR

T1 - GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - the KAGRA Collaboration

AU - Abbott, R.

AU - Adya, V. B.

AU - Bose, S.

AU - Brandt, J.

AU - Brown, D. D.

AU - Chatterjee, C.

AU - Chen, X.

AU - Chen, Y.-B.

AU - Chen, Y.-R.

AU - Cheng, H.

AU - Choudhary, R. K.

AU - Danilishin, S.

AU - Danzmann, K.

AU - Guo, H.-K.

AU - Hansen, H.

AU - Hennig, J.

AU - Heurs, M.

AU - Hreibi, A.

AU - Hübner, M. T.

AU - Isleif, K.

AU - Lang, R. N.

AU - Lee, H. K.

AU - Lee, H. M.

AU - Lee, H. M.

AU - Lee, J.

AU - Lehmann, J.

AU - Li, J.

AU - Li, X.

AU - Lück, H.

AU - More, A.

AU - Nguyen, T.

AU - Richardson, L.

AU - Rose, C. A.

AU - Roy, S.

AU - Sanders, J. R.

AU - Schmidt, P.

AU - Schmidt, S.

AU - Sun, L.

AU - Vahlbruch, H.

AU - Wilken, D.

AU - Willke, B.

AU - Wu, D. S.

AU - Wu, H.

AU - Yamamoto, Kohei

AU - Zhang, H.

AU - Zhang, L.

AU - Zhang, Y.

AU - Zheng, Y.

AU - Zhou, Z.

AU - Zhu, X. J.

AU - Affeldt, C.

AU - Bergamin, F.

AU - Bisht, A.

AU - Bode, N.

AU - Booker, P.

AU - Brinkmann, M.

AU - Gohlke, N.

AU - Heidt, A.

AU - Heinze, J.

AU - Hochheim, S.

AU - Kastaun, W.

AU - Kirchhoff, R.

AU - Koch, P.

AU - Koper, N.

AU - Kringel, V.

AU - Krishnendu, N. V.

AU - Kuehn, G.

AU - Leavey, S.

AU - Liu, J.

AU - Lough, J. D.

AU - Matiushechkina, M.

AU - Mehmet, M.

AU - Meylahn, F.

AU - Mukund, Nikhil

AU - Nadji, S. L.

AU - Nery, M.

AU - Ohme, F.

AU - Schneewind, M.

AU - Schulte, B. W.

AU - Schutz, B. F.

AU - Venneberg, J.

AU - von Wrangel, J.

AU - Weinert, M.

AU - Wellmann, F.

AU - Weßels, P.

AU - Winkler, W.

AU - Woehler, J.

AU - Junker, Jonas

PY - 2023/12/4

Y1 - 2023/12/4

N2 - 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 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 \(p_\mathrm{astro} > 0.5\). 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 \(p_\mathrm{astro} > 0.5\) 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 \(p_\mathrm{astro} > 0.5\) 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.

AB - 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 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 \(p_\mathrm{astro} > 0.5\). 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 \(p_\mathrm{astro} > 0.5\) 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 \(p_\mathrm{astro} > 0.5\) 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.

KW - gr-qc

KW - astro-ph.HE

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U2 - 10.1103/PhysRevX.13.041039

DO - 10.1103/PhysRevX.13.041039

M3 - Article

VL - 13

JO - Physical Review X

JF - Physical Review X

SN - 2160-3308

IS - 4

M1 - 041039

ER -

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