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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

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
Authors:	Soares-Santos M; Palmese A; Hartley W; Annis J; Garcia-Bellido J; Lahav O; Doctor Z; Fishbach M; Holz DE; Lin H; Pereira MES; Garcia A; Herner K; Kessler R; Peiris HV; Sako M; Allam S; Brout D; Rosell AC; Chen HY; Conselice C; deRose J; deVicente J; Diehl HT; Gill MSS; Gschwend J; Sevilla-Noarbe I; Tucker DL; Wechsler R; Berger E; Cowperthwaite PS; Metzger BD; Williams PKG; Abbott TMC; Abdalla FB; Avila S; Bechtol K; Bertin E; Brooks D; Buckley-Geer E; Burke DL; Kind MC; Carretero J; Castander FJ; Crocce M; Cunha CE; D'Andrea CB; da Costa LN; Davis C; Desai S; Doel P; Drlica-Wagner A; Eifler TF; Evrard AE; Flaugher B; Fosalba P; Frieman J; Gaztanaga E; Gerdes DW; Gruen D; Gruendl RA; Gutierrez G; Hollowood DL; Hoyle B; James DJ; Jeltema T; Kuehn K; Kuropatkin N; Li TS; Lima M; Maia MAG; Marshall JL; Menanteau F; Miquel R; Neilsen E; Ogando RLC; Plazas AA; Romer AK; Roodman A; Sanchez E; Scarpine V; Schindler R; Schubnell M; Serrano S; Smith M; Smith RC; Sobreira F; Suchyta E; Swanson MEC; Tarle G; Thomas RC; Walker AR; Wester W; Zuntz J; Abbott BP; Abbott R; Abbott TD; Abraham S; Acernese F; Ackley K; Adams C; Adhikari RX; Adya VB; Affeldt C; Agathos M; Agatsuma K; Aggarwal N; Aguiar OD; Aiello L; Ain A; Ajith P; Allen G; Allocca A; Aloy MA; Altin PA; Amato A; Ananyeva A; Anderson SB; Anderson WG; Angelova SV; Appert S; Arai K; Araya MC; Areeda JS; Arene M; Ascenzi S; Ashton G; Aston SM; Astone P; Aubin F; Aufmuth P; AultONeal K; Austin C; Avendano V; Avila-Alvarez A; Babak S; Bacon P; Badaracco F; Bader MKM; Bae S; Baker PT; Baldaccini F; Ballardin G; Ballmer SW; Banagiri S; Barayoga JC; Barclay SE; Barish BC; Barker D; Barkett K; Barnum S; Barone F; Barr B; Barsotti L; Barsuglia M; Barta D; Bartlett J; Bartos I; Bassiri R; Basti A; Bawaj M; Bayley JC; Bazzan M; Becsy B; Bejger M; Bell AS; Beniwal D; Bergmann G; Bernuzzi S; Bero JJ; Berry CPL; Bersanetti D; Bertolini A; Betzwieser J; Bhandare R; Bidler J; Bilenko IA; Bilgili SA; Billingsley G; Birch J; Birney R; Birnholtz O; Biscans S; Biscoveanu S; Bisht A; Bitossi M; Blackburn JK; Blair CD; Blair DG; Blair RM; Bloemen S; Bode N; Boer M; Boetzel Y; Bogaert G; Bondu F; Bonilla E; Bonnand R; Booker P; Boom BA; Booth CD; Bork R; Boschi V; Bose S; Bossie K; Bossilkov V; Bosveld J; Bouffanais Y; Bozzi A; Bradaschia C; Brady PR; Bramley A; Branchesi M; Brau JE; Briant T; Briggs JH; Brighenti F; Brillet A; Brinkmann M; Brockill P; Brooks AF; Brown DD; Brunett S; Buikema A; Bulik T; Bulten HJ; Buonanno A; Buskulic D; Buy C; Byer RL; Cabero M; Cadonati L; Cagnoli G; Cahillane C; Bustillo JC; Callister TA; Calloni E; Camp JB; Campbell WA; Cannon KC; Cao H; Cao J; Capocasa E; Carbognani F; Caride S; Carney MF; Carullo G; Diaz JC; Casentini C; Caudill S; Cavaglia M; Cavalieri R; Cella G; Cerda-Duran P; Cerretani G; Cesarini E; Chaibi O; Chakravarti K; Chamberlin SJ; Chan M; Chao S; Charlton P; Chase EA; Chassande-Mottin E; Chatterjee D; Chaturvedi M; Chatziioannou K; Cheeseboro BD; Chen X; Chen Y; Cheng HP; 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Hulko M; Husa S; Huttner SH; Huynh-Dinh T; Idzkowski B; Iess A; Ingram C; Inta R; Intini G; Irwin B; Isac JM; Isa HN; Isi M; Iyer BR; Izumi K; Jacqmin T; Jadhav SJ; Jani K; Janthalur NN; Jaranowski P; Jenkins AC; Jiang J; Johnson DS; Jones AW; Jones DI; Jones R; Jonker RJG; Ju L; Junker J; Kalaghatgi CV; Kalogera V; Kamai B; Kandhasamy S; Kang G; Kanner JB; Kapadia SJ; Karki S; Karvinen KS; Kashyap R; Kasprzack M; Katsanevas S; Katsavounidis E; Katzman W; Kaufer S; Kawabe K; Keerthana NV; Kefelian F; Keitel D; Kennedy R; Key JS; Khalili FY; Khan H; Khan I; Khan S; Khan Z; Khazanov EA; Khursheed M; Kijbunchoo N; Kim C; Kim JC; Kim K; Kim YM; Kim W; Kim WS; Kimball C; King EJ; King PJ; Kinley-Hanlon M; Kirchhoff R; Kissel JS; Kleybolte L; Klika JH; Klimenko S; Knowles TD; Koch P; Koehlenbeck SM; Koekoek G; Koley S; Kondrashov V; Kontos A; Koper N; Korobko M; Korth WZ; Kowalska I; Kozak DB; Kringel V; Krishnendu N; Krolak A; Kuehn G; Kumar A; Kumar P; Kumar R; Kumar S; Kuo L; Kutynia A; Kwang S; 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Contributors:	Soares-Santos, M; Palmese, A; Hartley, W; Annis, J; Garcia-Bellido, J; Lahav, O; Doctor, Z; Fishbach, M; Holz, De; Lin, H; Pereira, Me; Garcia, A; Herner, K; Kessler, R; Peiris, Hv; Sako, M; Allam, S; Brout, D; Rosell, Ac; Chen, Hy; Conselice, C; Derose, J; Devicente, J; Diehl, Ht; Gill, M; Gschwend, J; Sevilla-Noarbe, I; Tucker, Dl; Wechsler, R; Berger, E; Cowperthwaite, P; Metzger, Bd; Williams, Pkg; Abbott, Tmc; Abdalla, Fb; Avila, S; Bechtol, K; Bertin, E; Brooks, D; Buckley-Geer, E; Burke, Dl; Kind, Mc; Carretero, J; Castander, Fj; Crocce, M; Cunha, Ce; D'Andrea, Cb; da Costa, Ln; Davis, C; Desai, S; Doel, P; Drlica-Wagner, A; Eifler, Tf; Evrard, Ae; Flaugher, B; Fosalba, P; Frieman, J; Gaztanaga, E; Gerdes, Dw; Gruen, D; Gruendl, Ra; Gutierrez, G; Hollowood, Dl; Hoyle, B; James, Dj; Jeltema, T; Kuehn, K; Kuropatkin, N; Li, T; Lima, M; Maia, Mag; Marshall, Jl; Menanteau, F; Miquel, R; Neilsen, E; Ogando, Rlc; Plazas, Aa; Romer, Ak; Roodman, A; Sanchez, E; Scarpine, V; Schindler, R; Schubnell, M; Serrano, S; Smith, M; Smith, Rc; Sobreira, F; Suchyta, E; Swanson, Mec; Tarle, G; Thomas, Rc; Walker, Ar; Wester, W; Zuntz, J; Abbott, Bp; Abbott, R; Abbott, Td; Abraham, S; Acernese, F; Ackley, K
Publication Year:	2019
Collection:	Università degli studi di Trieste: ArTS (Archivio della ricerca di Trieste)
Subject Terms:	catalog; cosmology: observation; gravitational wave; surveys
Description:	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 H-0 = 75(-32)(+40) km s(-1) Mpc(-1) , 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 H-0 = 78(-24)(+96) km s(-1) Mpc(-1) (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.
Document Type:	article in journal/newspaper
Language:	English
Relation:	info:eu-repo/semantics/altIdentifier/wos/WOS:000466274600004; volume:876; issue:1; firstpage:1; lastpage:15; numberofpages:15; journal:THE ASTROPHYSICAL JOURNAL LETTERS; https://hdl.handle.net/11368/3003335
DOI:	10.3847/2041-8213/ab14f1
Availability:	https://hdl.handle.net/11368/3003335; https://doi.org/10.3847/2041-8213/ab14f1
Rights:	info:eu-repo/semantics/openAccess
Accession Number:	edsbas.34ECE671
Database:	BASE