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

被引：198

作者：

Soares-Santos, M. ^{[1
]}

Palmese, A. ^{[2
]}

Hartley, W. ^{[3
]}

Annis, J. ^{[2
]}

Garcia-Bellido, J. ^{[4
]}

Lahav, O. ^{[3
]}

Doctor, Z. ^{[5
,6
]}

Fishbach, M. ^{[6
]}

Holz, D. E. ^{[7
]}

Lin, H. ^{[2
]}

Pereira, M. E. S. ^{[1
]}

Garcia, A. ^{[1
,80
]}

Herner, K. ^{[2
]}

Kessler, R. ^{[6
,8
]}

Peiris, H., V ^{[3
]}

Sako, M. ^{[9
]}

Allam, S. ^{[2
]}

Brout, D. ^{[9
]}

Carnero Rosell, A. ^{[10
,11
]}

Chen, H. Y. ^{[7
]}

Conselice, C. ^{[12
]}

deRose, J. ^{[13
,14
,15
]}

deVicente, J. ^{[10
]}

Diehl, H. T. ^{[2
]}

Gill, M. S. S. ^{[16
]}

Gschwend, J. ^{[11
,17
]}

Sevilla-Noarbe, I ^{[10
]}

Tucker, D. L. ^{[2
]}

Wechsler, R. ^{[16
,18
,19
]}

Berger, E. ^{[20
]}

Cowperthwaite, P. S. ^{[21
]}

Metzger, B. D. ^{[22
]}

Williams, P. K. G. ^{[20
,23
]}

Abbott, T. M. C. ^{[24
]}

Abdalla, F. B. ^{[3
]}

Avila, S. ^{[25
]}

Bechtol, K. ^{[26
,27
]}

Bertin, E. ^{[28
,29
]}

Brooks, D. ^{[3
]}

Buckley-Geer, E. ^{[2
]}

Burke, D. L. ^{[16
,19
]}

Kind, M. Carrasco ^{[30
,31
]}

Carretero, J. ^{[32
]}

Castander, F. J. ^{[33
,34
]}

Crocce, M. ^{[33
,34
]}

Cunha, C. E. ^{[19
]}

D'Andrea, C. B. ^{[9
]}

da Costa, L. N. ^{[11
,17
]}

Davis, C. ^{[19
]}

Desai, S. ^{[35
]}

机构：

[1] Brandeis Univ, Dept Phys, Waltham, MA 02453 USA

[2] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[3] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[4] Univ Autonoma Madrid, Inst Fis Teor, CSIC, E-28049 Madrid, Spain

[5] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[6] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[7] Univ Chicago, Chicago, IL 60637 USA

[8] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA

[9] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[10] CIEMAT, Madrid, Spain

[11] Lab Interinst e Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[12] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England

[13] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[14] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[15] SLAC Natl Accelerator Lab, Dept Particle Phys & Astrophys, Menlo Pk, CA 94025 USA

[16] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[17] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[18] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[19] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[20] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[21] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA

[22] Columbia Univ, Dept Phys, New York, NY 10025 USA

[23] Amer Astron Soc, 1667 K St NW,Suite 800, Washington, DC 20006 USA

[24] Natl Opt Astron Observ, Cerro Tololo Inter Amer Observ, La Serena 603, Chile

[25] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[26] LSST, 933 North Cherry Ave, Tucson, AZ 85721 USA

[27] Univ Wisconsin, Phys Dept, 2320 Chamberlin Hall,1150 Univ Ave, Madison, WI 53706 USA

[28] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[29] UPMC Univ Paris 06, Sorbonne Univ, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[30] Univ Illinois, Dept Astron, 1002 West Green St, Urbana, IL 61801 USA

[31] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA

[32] Barcelona Inst Sci & Technol, IFAE, Campus UAB, E-08193 Bellaterra, Barcelona, Spain

[33] Inst Estudis Espacials Catalunya, E-08034 Barcelona, Spain

[34] CSIC, Inst Space Sci, Campus UAB,Caner Can Magrans S-N, E-08193 Barcelona, Spain

[35] IIT Hyderabad, Dept Phys, Kandi 502285, Telangana, India

[36] Steward Observ, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA

[37] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[38] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[39] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[40] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[41] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany

[42] Univ Sternwarte, Ludwig Maximilians Univ Munchen, Fak Phys, Scheinerstr 1, D-81679 Munich, Germany

[43] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[44] Macquarie Univ, Australian Astron Opt, N Ryde, NSW 2113, Australia

[45] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, CP 66318, BR-05314970 Sao Paulo, SP, Brazil

[46] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA

[47] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[48] Inst Catalana Recerca & Estudis Avancats, E-08010 Barcelona, Spain

[49] Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA

[50] Univ Sussex, Dept Phys & Astron, Pevensey Bldg, Brighton BN1 9QH, E Sussex, England

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2019年 / 876卷 / 01期

基金：

俄罗斯基础研究基金会; 瑞士国家科学基金会; 俄罗斯科学基金会; 匈牙利科学研究基金会; 澳大利亚研究理事会; 美国国家科学基金会; 英国工程与自然科学研究理事会; 新加坡国家研究基金会; 英国科学技术设施理事会; 中国国家自然科学基金;

关键词：

catalogs; cosmology: observations; gravitational waves; surveys; STELLAR MASS; RESOLUTION; CATALOG;

D O I：

10.3847/2041-8213/ab14f1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：15

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