A Statistical Standard Siren Measurement of the Hubble Constant from the LIGO/Virgo Gravitational Wave Compact Object Merger GW190814 and Dark Energy Survey Galaxies,The Astrophysical Journal Letters

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A Statistical Standard Siren Measurement of the Hubble Constant from the LIGO/Virgo Gravitational Wave Compact Object Merger GW190814 and Dark Energy Survey Galaxies
The Astrophysical Journal Letters ( IF 8.8 ) Pub Date : 2020-09-06 , DOI: 10.3847/2041-8213/abaeff
A. Palmese _{1,

2} , J. deVicente ₃ , M. E. S. Pereira ₄ , J. Annis ₁ , W. Hartley _{5,

6,

7} , K. Herner ₁ , M. Soares-Santos ₄ , M. Crocce _{8,

9} , D. Huterer ₁₀ , I. Magaa Hernandez ₁₁ , A. Garcia ₄ , J. Garcia-Bellido ₁₂ , J. Gschwend _{13,

14} , D. E. Holz ₂ , R. Kessler _{2,

15} , O. Lahav ₆ , R. Morgan ₁₆ , C. Nicolaou ₆ , C. Conselice ₁₇ , R. J. Foley ₁₈ , M. S. S. Gill ₁₉ , T. M. C. Abbott ₂₀ , M. Aguena _{13,

21} , S. Allam ₁ , S. Avila ₁₂ , K. Bechtol ₁₆ , E. Bertin _{22,

23} , S. Bhargava ₂₄ , D. Brooks ₆ , E. Buckley-Geer ₁ , D. L. Burke _{19,

25} , M. Carrasco Kind _{26,

27} , J. Carretero ₂₈ , F. J. Castander _{8,

9} , C. Chang _{2,

15} , M. Costanzi _{29,

30} , L. N. da Costa _{13,

14} , T. M. Davis ₃₁ , S. Desai ₃₂ , H. T. Diehl ₁ , P. Doel ₆ , A. Drlica-Wagner _{1,

2,

15} , J. Estrada ₁ , S. Everett ₁₈ , A. E. Evrard _{10,

33} , E. Fernandez ₂₈ , D. A. Finley ₁ , B. Flaugher ₁ , P. Fosalba _{8,

9} , J. Frieman _{1,

2} , E. Gaztanaga _{8,

9} , D. W. Gerdes _{10,

33} , D. Gruen _{19,

25,

34} , R. A. Gruendl _{26,

27} , G. Gutierrez ₁ , S. R. Hinton ₃₁ , D. L. Hollowood ₁₈ , K. Honscheid _{35,

36} , D. J. James ₃₇ , S. Kent _{1,

2} , E. Krause ₃₈ , K. Kuehn _{39,

40} , H. Lin ₁ , M. A. G. Maia _{13,

14} , M. March ₄₁ , J. L. Marshall ₄₂ , P. Melchior ₄₃ , F. Menanteau _{26,

27} , R. Miquel _{28,

44} , R. L. C. Ogando _{13,

14} , F. Paz-Chinchn _{27,

45} , A. A. Plazas ₄₃ , A. Roodman _{19,

25} , M. Sako ₄₁ , E. Sanchez ₃ , V. Scarpine ₁ , M. Schubnell ₁₀ , S. Serrano _{8,

9} , I. Sevilla-Noarbe ₃ , J. Allyn. Smith ₄₆ , M. Smith ₄₇ , E. Suchyta ₄₈ , G. Tarle ₁₀ , M. A. Troxel ₄₉ , D. L. Tucker ₁ , A. R. Walker ₂₀ , W. Wester ₁ , R. D. Wilkinson ₂₄ , J. Zuntz ₅₀

Affiliation

Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510, USA
Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
Centro de Investigaciones Energticas, Medioambientales y Tecnolgicas (CIEMAT), Madrid, Spain
Department of Physics, Brandeis University, Waltham, MA 02453, USA
Dpartement de Physique Thorique and Center for Astroparticle Physics, Universit de Genve, 24 quai Ernest Ansermet, CH-1211 Geneva, Switzerland
Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain
Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
University of Wisconsin-Milwaukee, Milwaukee, WI 53201, USA
Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
Laboratrio Interinstitucional de e-Astronomia—LIneA, Rua Gal. Jos Cristino 77, Rio de Janeiro, RJ—20921-400, Brazil
Observatrio Nacional, Rua Gal. Jos Cristino 77, Rio de Janeiro, RJ—20921-400, Brazil
Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA
Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, WI 53706-1390, USA
University of Nottingham, School of Physics and Astronomy, Nottingham NG7 2RD, UK
Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Cerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
Departamento de Fsica Matemtica, Instituto de Fsica, Universidade de So Paulo, CP 66318, Sao Paulo, SP, 05314-970, Brazil
CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France
Sorbonne Universits, UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France
Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, UK
Kavli Institute for Particle Astrophysics & Cosmology, P.O. Box 2450, Stanford University, Stanford, CA 94305, USA
Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA
National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, IL 61801, USA
Institut de Fsica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
INAF-Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, I-34143 Trieste, Italy
Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy
School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA
Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA
Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
Department of Physics, The Ohio State University, Columbus, OH 43210, USA
Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA
Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia
Lowell Observatory, 1400 Mars Hill Road, Flagstaff, AZ 86001, USA
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
Instituci Catalana de Recerca i Estudis Avanats, E-08010 Barcelona, Spain
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Austin Peay State University, Dept. Physics, Engineering and Astronomy, P.O. Box 4608 Clarksville, TN 37044, USA
School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK
Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
Department of Physics, Duke University Durham, NC 27708, USA
Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, UK

We present a measurement of the Hubble constant H 0 using the gravitational wave (GW) event GW190814, which resulted from the coalescence of a 23 M ⊙ black hole with a 2.6 M ⊙ compact object, as a standard siren. No compelling electromagnetic counterpart has been identified for this event; thus our analysis accounts for thousands of potential host galaxies within a statistical framework. The redshift information is obtained from the photometric redshift (photo- z ) catalog from the Dark Energy Survey. The luminosity distance is provided by the LIGO/Virgo gravitational wave sky map. Since this GW event has the second-smallest localization volume after GW170817, GW190814 is likely to provide the best constraint on cosmology from a single standard siren without identifying an electromagnetic counterpart. Our analysis uses photo- z probability distribution functions and corrects for photo- z biases. We also reana...

中文翻译：

LIGO /处女座引力波紧凑物体合并GW190814和暗能量调查星系对哈勃常数的统计标准警笛测量

我们使用引力波（GW）事件GW190814给出了对哈勃常数H 0的测量，该事件是由23 M⊙黑洞与2.6 M M紧凑物体作为标准警报器合并而成的。尚未发现与此事件相关的引人注目的电磁对手；因此，我们的分析在一个统计框架内解释了数千个潜在的宿主星系。红移信息是从“暗能量调查”的光度红移（photo-z）目录中获得的。亮度距离由LIGO /处女座引力波天空图提供。由于此GW事件的定位量仅次于GW170817，仅次于GW170，因此GW190814可能会在不识别电磁对等物的情况下，从单个标准警报器提供对宇宙学的最佳约束。我们的分析使用了photoz概率分布函数并校正了photoz偏差。我们还重新

更新日期：2020-09-08

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