First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Autoren

  • DES Collaboration
  • The LIGO Scientific Collaboration
  • Virgo Collaboration
  • V. B. Adya
  • S. L. Danilishin
  • K. Danzmann
  • M. Heurs
  • A. Hreibi
  • H. Lück
  • D. Steinmeyer
  • H. Vahlbruch
  • L.-w. Wei
  • D. M. Wilken
  • B. Willke
  • H. Wittel
  • Christoph Affeldt
  • Peter Aufmuth
  • Gerald Bergmann
  • Aparna Bisht
  • Nina Bode
  • P. Booker
  • Marc Brinkmann
  • M. Cabero
  • T. Dent
  • O. de Varona
  • S. Doravari
  • S. Hochheim
  • J. Junker
  • Kai S. Karvinen
  • Stefan Kaufer
  • S. Khan
  • R. Kirchhoff
  • Patrick Koch
  • S. M. Köhlenbeck
  • Volker Kringel
  • N. Koper
  • G. Kuehn
  • S. Leavey
  • J. Lehmann
  • James Lough
  • Moritz Mehmet
  • M. Nery
  • F. Ohme
  • P. Oppermann
  • M. Phelps
  • O. Puncken
  • A. Rüdiger
  • Emil Schreiber
  • B. W. Schulte
  • M. Standke
  • M. Steinke
  • Fabian Thies
  • F. Wellmann
  • Peter Weßels
  • Maximilian H. Wimmer
  • W. Winkler
  • J. Woehler
  • M. M. Hanke
  • J. Hennig
  • Mukherjee Arunava Mukherjee
  • Michael Weinert

Organisationseinheiten

Externe Organisationen

  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • Tata Institute of Fundamental Research (TIFR HYD)
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
AufsatznummerL7
Seitenumfang15
FachzeitschriftAstrophysical Journal Letters
Jahrgang876
Ausgabenummer1
PublikationsstatusVeröffentlicht - 26 Apr. 2019

Abstract

We present a multi-messenger measurement of the Hubble constant H 0 using the binary-black-hole merger GW170814 as a standard siren, combined with a photometric redshift catalog from the Dark Energy Survey (DES). The luminosity distance is obtained from the gravitational wave signal detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo Collaboration (LVC) on 2017 August 14, and the redshift information is provided by the DES Year 3 data. Black hole mergers such as GW170814 are expected to lack bright electromagnetic emission to uniquely identify their host galaxies and build an object-by-object Hubble diagram. However, they are suitable for a statistical measurement, provided that a galaxy catalog of adequate depth and redshift completion is available. Here we present the first Hubble parameter measurement using a black hole merger. Our analysis results in , which is consistent with both SN Ia and cosmic microwave background measurements of the Hubble constant. The quoted 68% credible region comprises 60% of the uniform prior range [20, 140] km s -1 Mpc -1, and it depends on the assumed prior range. If we take a broader prior of [10, 220] km s -1 Mpc -1, we find (57% of the prior range). Although a weak constraint on the Hubble constant from a single event is expected using the dark siren method, a multifold increase in the LVC event rate is anticipated in the coming years and combinations of many sirens will lead to improved constraints on H 0.

ASJC Scopus Sachgebiete

Zitieren

First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814. / DES Collaboration; The LIGO Scientific Collaboration; Virgo Collaboration et al.
in: Astrophysical Journal Letters, Jahrgang 876, Nr. 1, L7, 26.04.2019.

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

DES Collaboration, The LIGO Scientific Collaboration, Virgo Collaboration, Adya, VB, Danilishin, SL, Danzmann, K, Heurs, M, Hreibi, A, Lück, H, Steinmeyer, D, Vahlbruch, H, Wei, L, Wilken, DM, Willke, B, Wittel, H, Affeldt, C, Aufmuth, P, Bergmann, G, Bisht, A, Bode, N, Booker, P, Brinkmann, M, Cabero, M, Dent, T, de Varona, O, Doravari, S, Hochheim, S, Junker, J, Karvinen, KS, Kaufer, S, Khan, S, Kirchhoff, R, Koch, P, Köhlenbeck, SM, Kringel, V, Koper, N, Kuehn, G, Leavey, S, Lehmann, J, Lough, J, Mehmet, M, Nery, M, Ohme, F, Oppermann, P, Phelps, M, Puncken, O, Rüdiger, A, Schreiber, E, Schulte, BW, Standke, M, Steinke, M, Thies, F, Wellmann, F, Weßels, P, Wimmer, MH, Winkler, W, Woehler, J, Hanke, MM, Hennig, J, Arunava Mukherjee, M & Weinert, M 2019, 'First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814', Astrophysical Journal Letters, Jg. 876, Nr. 1, L7. https://doi.org/10.3847/2041-8213/ab14f1
DES Collaboration, The LIGO Scientific Collaboration, Virgo Collaboration, Adya, V. B., Danilishin, S. L., Danzmann, K., Heurs, M., Hreibi, A., Lück, H., Steinmeyer, D., Vahlbruch, H., Wei, L., Wilken, D. M., Willke, B., Wittel, H., Affeldt, C., Aufmuth, P., Bergmann, G., Bisht, A., ... Weinert, M. (2019). First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814. Astrophysical Journal Letters, 876(1), Artikel L7. https://doi.org/10.3847/2041-8213/ab14f1
DES Collaboration, The LIGO Scientific Collaboration, Virgo Collaboration, Adya VB, Danilishin SL, Danzmann K et al. First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814. Astrophysical Journal Letters. 2019 Apr 26;876(1):L7. doi: 10.3847/2041-8213/ab14f1
Download
@article{bd1e8aa7a2934a37b41450475eadffd2,
title = "First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814",
abstract = "We present a multi-messenger measurement of the Hubble constant H 0 using the binary-black-hole merger GW170814 as a standard siren, combined with a photometric redshift catalog from the Dark Energy Survey (DES). The luminosity distance is obtained from the gravitational wave signal detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo Collaboration (LVC) on 2017 August 14, and the redshift information is provided by the DES Year 3 data. Black hole mergers such as GW170814 are expected to lack bright electromagnetic emission to uniquely identify their host galaxies and build an object-by-object Hubble diagram. However, they are suitable for a statistical measurement, provided that a galaxy catalog of adequate depth and redshift completion is available. Here we present the first Hubble parameter measurement using a black hole merger. Our analysis results in , which is consistent with both SN Ia and cosmic microwave background measurements of the Hubble constant. The quoted 68% credible region comprises 60% of the uniform prior range [20, 140] km s -1 Mpc -1, and it depends on the assumed prior range. If we take a broader prior of [10, 220] km s -1 Mpc -1, we find (57% of the prior range). Although a weak constraint on the Hubble constant from a single event is expected using the dark siren method, a multifold increase in the LVC event rate is anticipated in the coming years and combinations of many sirens will lead to improved constraints on H 0. ",
author = "{DES Collaboration} and {The LIGO Scientific Collaboration} and {The Virgo Collaboration} and M. Soares-santos and A. Palmese and W. Hartley and J. Annis and J. Garcia-bellido and O. Lahav and Z. Doctor and M. Fishbach and Holz, {D. E.} and H. Lin and Pereira, {M. E. S.} and A. Garcia and K. Herner and R. Kessler and Peiris, {H. V.} and M. Sako and S. Allam and D. Brout and Rosell, {A. Carnero} and Chen, {H. Y.} and C. Conselice and J. Derose and J. Devicente and Diehl, {H. T.} and Gill, {M. S. S.} and J. Gschwend and I. Sevilla-noarbe and Tucker, {D. L.} and R. Wechsler and E. Berger and Cowperthwaite, {P. S.} and Metzger, {B. D.} and Williams, {P. K. G.} and Abbott, {T. M. C.} and Abdalla, {F. B.} and S. Avila and K. Bechtol and E. Bertin and Adya, {V. B.} and Danilishin, {S. L.} and K. Danzmann and M. Heurs and A. Hreibi and H. L{\"u}ck and D. Steinmeyer and H. Vahlbruch and L.-w. Wei and Wilken, {D. M.} and B. Willke and H. Wittel and Christoph Affeldt and Peter Aufmuth and Gerald Bergmann and Aparna Bisht and Nina Bode and P. Booker and Marc Brinkmann and M. Cabero and T. Dent and {de Varona}, O. and S. Doravari and S. Hochheim and J. Junker and Karvinen, {Kai S.} and Stefan Kaufer and S. Khan and R. Kirchhoff and Patrick Koch and K{\"o}hlenbeck, {S. M.} and Volker Kringel and N. Koper and G. Kuehn and S. Leavey and J. Lehmann and James Lough and Moritz Mehmet and M. Nery and F. Ohme and P. Oppermann and M. Phelps and O. Puncken and A. R{\"u}diger and Emil Schreiber and Schulte, {B. W.} and M. Standke and M. Steinke and Fabian Thies and F. Wellmann and Peter We{\ss}els and Wimmer, {Maximilian H.} and W. Winkler and J. Woehler and Hanke, {M. M.} and J. Hennig and {Arunava Mukherjee}, Mukherjee and Michael Weinert",
year = "2019",
month = apr,
day = "26",
doi = "10.3847/2041-8213/ab14f1",
language = "English",
volume = "876",
journal = "Astrophysical Journal Letters",
issn = "2041-8205",
publisher = "IOP Publishing Ltd.",
number = "1",

}

Download

TY - JOUR

T1 - First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814

AU - DES Collaboration

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Soares-santos, M.

AU - Palmese, A.

AU - Hartley, W.

AU - Annis, J.

AU - Garcia-bellido, J.

AU - Lahav, O.

AU - Doctor, Z.

AU - Fishbach, M.

AU - Holz, D. E.

AU - Lin, H.

AU - Pereira, M. E. S.

AU - Garcia, A.

AU - Herner, K.

AU - Kessler, R.

AU - Peiris, H. V.

AU - Sako, M.

AU - Allam, S.

AU - Brout, D.

AU - Rosell, A. Carnero

AU - Chen, H. Y.

AU - Conselice, C.

AU - Derose, J.

AU - Devicente, J.

AU - Diehl, H. T.

AU - Gill, M. S. S.

AU - Gschwend, J.

AU - Sevilla-noarbe, I.

AU - Tucker, D. L.

AU - Wechsler, R.

AU - Berger, E.

AU - Cowperthwaite, P. S.

AU - Metzger, B. D.

AU - Williams, P. K. G.

AU - Abbott, T. M. C.

AU - Abdalla, F. B.

AU - Avila, S.

AU - Bechtol, K.

AU - Bertin, E.

AU - Adya, V. B.

AU - Danilishin, S. L.

AU - Danzmann, K.

AU - Heurs, M.

AU - Hreibi, A.

AU - Lück, H.

AU - Steinmeyer, D.

AU - Vahlbruch, H.

AU - Wei, L.-w.

AU - Wilken, D. M.

AU - Willke, B.

AU - Wittel, H.

AU - Affeldt, Christoph

AU - Aufmuth, Peter

AU - Bergmann, Gerald

AU - Bisht, Aparna

AU - Bode, Nina

AU - Booker, P.

AU - Brinkmann, Marc

AU - Cabero, M.

AU - Dent, T.

AU - de Varona, O.

AU - Doravari, S.

AU - Hochheim, S.

AU - Junker, J.

AU - Karvinen, Kai S.

AU - Kaufer, Stefan

AU - Khan, S.

AU - Kirchhoff, R.

AU - Koch, Patrick

AU - Köhlenbeck, S. M.

AU - Kringel, Volker

AU - Koper, N.

AU - Kuehn, G.

AU - Leavey, S.

AU - Lehmann, J.

AU - Lough, James

AU - Mehmet, Moritz

AU - Nery, M.

AU - Ohme, F.

AU - Oppermann, P.

AU - Phelps, M.

AU - Puncken, O.

AU - Rüdiger, A.

AU - Schreiber, Emil

AU - Schulte, B. W.

AU - Standke, M.

AU - Steinke, M.

AU - Thies, Fabian

AU - Wellmann, F.

AU - Weßels, Peter

AU - Wimmer, Maximilian H.

AU - Winkler, W.

AU - Woehler, J.

AU - Hanke, M. M.

AU - Hennig, J.

AU - Arunava Mukherjee, Mukherjee

AU - Weinert, Michael

PY - 2019/4/26

Y1 - 2019/4/26

N2 - We present a multi-messenger measurement of the Hubble constant H 0 using the binary-black-hole merger GW170814 as a standard siren, combined with a photometric redshift catalog from the Dark Energy Survey (DES). The luminosity distance is obtained from the gravitational wave signal detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo Collaboration (LVC) on 2017 August 14, and the redshift information is provided by the DES Year 3 data. Black hole mergers such as GW170814 are expected to lack bright electromagnetic emission to uniquely identify their host galaxies and build an object-by-object Hubble diagram. However, they are suitable for a statistical measurement, provided that a galaxy catalog of adequate depth and redshift completion is available. Here we present the first Hubble parameter measurement using a black hole merger. Our analysis results in , which is consistent with both SN Ia and cosmic microwave background measurements of the Hubble constant. The quoted 68% credible region comprises 60% of the uniform prior range [20, 140] km s -1 Mpc -1, and it depends on the assumed prior range. If we take a broader prior of [10, 220] km s -1 Mpc -1, we find (57% of the prior range). Although a weak constraint on the Hubble constant from a single event is expected using the dark siren method, a multifold increase in the LVC event rate is anticipated in the coming years and combinations of many sirens will lead to improved constraints on H 0.

AB - We present a multi-messenger measurement of the Hubble constant H 0 using the binary-black-hole merger GW170814 as a standard siren, combined with a photometric redshift catalog from the Dark Energy Survey (DES). The luminosity distance is obtained from the gravitational wave signal detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo Collaboration (LVC) on 2017 August 14, and the redshift information is provided by the DES Year 3 data. Black hole mergers such as GW170814 are expected to lack bright electromagnetic emission to uniquely identify their host galaxies and build an object-by-object Hubble diagram. However, they are suitable for a statistical measurement, provided that a galaxy catalog of adequate depth and redshift completion is available. Here we present the first Hubble parameter measurement using a black hole merger. Our analysis results in , which is consistent with both SN Ia and cosmic microwave background measurements of the Hubble constant. The quoted 68% credible region comprises 60% of the uniform prior range [20, 140] km s -1 Mpc -1, and it depends on the assumed prior range. If we take a broader prior of [10, 220] km s -1 Mpc -1, we find (57% of the prior range). Although a weak constraint on the Hubble constant from a single event is expected using the dark siren method, a multifold increase in the LVC event rate is anticipated in the coming years and combinations of many sirens will lead to improved constraints on H 0.

UR - http://www.scopus.com/inward/record.url?scp=85067276464&partnerID=8YFLogxK

U2 - 10.3847/2041-8213/ab14f1

DO - 10.3847/2041-8213/ab14f1

M3 - Article

VL - 876

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

SN - 2041-8205

IS - 1

M1 - L7

ER -

Von denselben Autoren

  1. Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo

    Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

  2. Ultralight vector dark matter search using data from the KAGRA O3GK run

    Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

  3. Quantum Enhanced Balanced Heterodyne Readout for Differential Interferometry

    Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

  4. Search for Gravitational-lensing Signatures in the Full Third Observing Run of the LIGO-Virgo Network

    Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

  5. Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M ⊙ Compact Object and a Neutron Star

    Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review