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Title: First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stz978· OSTI ID:1510042
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  1. Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
  2. Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
  3. School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
  4. ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Australia; The Research School of Astronomy and Astrophysics, Australian National University, ACT 2601, Australia
  5. African Institute for Mathematical Sciences, 6 Melrose Road, Muizenberg 7945, South Africa; South African Astronomical Observatory, P.O.Box 9, Observatory 7935, South Africa
  6. Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
  7. Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA; Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA
  8. Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA
  9. The Research School of Astronomy and Astrophysics, Australian National University, ACT 2601, Australia
  10. School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
  11. Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
  12. Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA
  13. Korea Astronomy and Space Science Institute, Yuseong-gu, Daejeon 305-348, Korea
  14. LSST, 933 North Cherry Avenue, Tucson, AZ 85721, USA
  15. Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
  16. 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
  17. Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, CA 94305, USA; SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
  18. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), E-28040 Madrid, Spain; Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
  19. INAF, Astrophysical Observatory of Turin, I-10025 Pino Torinese, Italy
  20. 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 St, Urbana, IL 61801, USA
  21. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
  22. 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
  23. Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, CA 94305, USA
  24. Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil; Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
  25. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), E-28040 Madrid, Spain
  26. Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA; Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA
  27. Department of Astronomy/Steward Observatory, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA
  28. Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA; Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
  29. Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA; Miller Institute for Basic Research in Science, University of California, Berkeley, CA 94720, USA
  30. Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
  31. PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA
  32. Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
  33. Centre for Astrophysics & Supercomputing, Swinburne University of Technology, VIC 3122, Australia
  34. CENTRA, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, P-1049-001 Lisboa, Portugal
  35. 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
  36. 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
  37. Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, D-85748 Garching, Germany; Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, D-81679 München, Germany
  38. Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
  39. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
  40. South African Astronomical Observatory, P.O.Box 9, Observatory 7935, South Africa; Department of Physics, University of Namibia, 340 Mandume Ndemufayo Avenue, Pionierspark, Windhoek 13301, Namibia
  41. Department of Astronomy/Steward Observatory, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA
  42. Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia
  43. Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW 2006, Australia
  44. Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil; Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318 São Paulo, SP 05314-970, Brazil
  45. Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA; Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA
  46. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain; Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
  47. Division of Theoretical Astronomy, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 10617, Taiwan
  48. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA
  49. Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, UK
  50. SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
  51. Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA
  52. Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil; Instituto de Física Gleb Wataghin, Universidade Estadual de Campinas, 13083-859 Campinas, SP, Brazil
  53. Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
  54. National Center for Supercomputing Applications, 1205 West Clark St, Urbana, IL 61801, USA
  55. Observatories of the Carnegie Institution for Science, 813 Santa Barbara St, Pasadena, CA 91101, USA
  56. Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439, USA

We propose an improved measurement of the Hubble Constant (H0) using the 'inverse distance ladder' method, which adds the information from 207 Type Ia supernovae (SNe Ia) from the Dark Energy Survey (DES) at redshift 0.018 < z < 0.85 to existing distance measurements of 122 low redshift (z < 0.07) SNe Ia (Low-z) and measurements of Baryon Acoustic Oscillations (BAOs). Whereas traditional measurements of H0 with SNe Ia use a distance ladder of parallax and Cepheid variable stars, the inverse distance ladder relies on absolute distance measurements from the BAOs to calibrate the intrinsic magnitude of the SNe Ia. We find H0 = 67.77 ± 1.3 km s-1 Mpc-1 (statistical and systematic uncertainties, 68% confidence). In this work, our measurement makes minimal assumptions about the underlying cosmological model, and our analysis was blinded to reduce confirmation bias. We investigate possible systematic uncertainties and all are presently below the statistical uncertainties. Our H0 value is consistent with estimates derived from the Cosmic Microwave Background assuming a ΔCDM universe (Planck Collaboration et al. 2018).

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
Contributing Organization:
DES Collaboration
Grant/Contract Number:
AC02-07CH11359; SC0007859; AC05-00OR22725; AC02-05CH11231; SC0019193
OSTI ID:
1510042
Alternate ID(s):
OSTI ID: 1531220; OSTI ID: 1561925; OSTI ID: 1646609; OSTI ID: 1725789
Report Number(s):
arXiv:1811.02376; FERMILAB-PUB-19-045-AE-CD; oai:inspirehep.net:1702373
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 2; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 122 works
Citation information provided by
Web of Science

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KiDS-450: testing extensions to the standard cosmological model journal April 2017
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CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA text January 2009
Model independent H(z) reconstruction using the cosmic inverse distance ladder text January 2019
Cosmography of f(R) gravity text January 2008
The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae text January 2009
The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae text January 2009
Hubble Residuals of Nearby Type Ia Supernovae Are Correlated with Host Galaxy Masses text January 2009
The Carnegie Supernova Project: Second Photometry Data Release of Low-Redshift Type Ia Supernovae text January 2011
New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75 text January 2012
CfA4: Light Curves for 94 Type Ia Supernovae text January 2012
A Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck text January 2013
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples text January 2013
Inflationary Freedom and Cosmological Neutrino Constraints text January 2014
Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs text January 2016
A 2.4% Determination of the Local Value of the Hubble Constant text January 2016
Reconciling CMB and structure growth measurements with dark energy interactions text January 2016
A cosmographic analysis of the transition to acceleration using SN-Ia and BAO text January 2016
Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature text January 2016
KiDS-450: Testing extensions to the standard cosmological model text January 2016
The need for accurate redshifts in supernova cosmology text January 2016
Dynamical dark energy in light of the latest observations text January 2017
The Carnegie Supernova Project I: Third Photometry Data Release of Low-Redshift Type Ia Supernovae and Other White Dwarf Explosions text January 2017
Improved constraints on H0 from a combined analysis of gravitational-wave and electromagnetic emission from GW170817 text January 2017
Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data text January 2017
New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant text January 2018
$H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method text January 2018
Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder text January 2018
H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant text January 2018
First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release text January 2018
Photometric redshifts from evolutionary synthesis with PEGASE: the code ZPEG and the z=0 age constraint text January 2002
Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler text January 2003
Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys text January 2003

Cited By (21)

Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data journal August 2019
The Hubble constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae journal August 2019
The Hubble–Lemaître constant and sound horizon from low-redshift probes journal May 2019
Constraints on the interacting vacuum–geodesic CDM scenario journal July 2019
A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging journal September 2019
Can redshift errors bias measurements of the Hubble Constant? journal September 2019
Observational constraints on interacting Tsallis holographic dark energy model journal September 2019
Current and Future Applications of Reverberation-Mapped Quasars in Cosmology journal December 2019
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM journal May 2019
A DECam Search for Explosive Optical Transients Associated with IceCube Neutrino Alerts journal September 2019
Calibrating the Cosmic Distance Ladder Using Gravitational-wave Observations journal November 2019
A Model-independent Determination of the Hubble Constant from Lensed Quasars and Supernovae Using Gaussian Process Regression journal November 2019
A DECam Search for Explosive Optical Transients Associated with IceCube Neutrinos text January 2019
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM text January 2019
Observational constraints on interacting Tsallis holographic dark energy models text January 2019
Local determination of the Hubble constant and the deceleration parameter text January 2019
A SHARP view of H0LiCOW: $H_{0}$ from three time-delay gravitational lens systems with adaptive optics imaging text January 2019
A DECam Search for Explosive Optical Transients Associated with IceCube Neutrinos text January 2019
Calibrating the cosmic distance ladder using gravitational-wave observations text January 2019
Can redshift errors bias measurements of the Hubble Constant? text January 2019
A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time text January 2020

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