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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogs for cosmological analysis

Authors :
Axel de la Macorra
Eric Jullo
Jeremy L. Tinker
J. N. McLane
Faizan G. Mohammad
Aurelio Carnero Rosell
Sylvain de la Torre
Hélion du Mas des Bourboux
Arnaud de Mattia
Peter Doohyun Choi
V. Ruhlmann-Kleider
Stephanie Escoffier
Hui Kong
S. Fromenteau
Stephen Bailey
Hee-Jong Seo
Solène Chabanier
Eva-Maria Mueller
Alex Smith
Jean-Paul Kneib
Joel R. Brownstein
Gong-Bo Zhao
Richard Neveux
Jonathan Brinkmann
Irene Cruz-González
Alexandra N. Higley
Kyle S. Dawson
Yucheng Zhang
Chia-Hsun Chuang
Andrea Muñoz-Gutiérrez
John Moustakas
Etienne Burtin
Johan Comparat
Will J. Percival
Christian Nitschelm
Shadab Alam
Donald P. Schneider
Graziano Rossi
Julian E. Bautista
Nathalie Palanque-Delabrouille
Anthony R. Pullen
Cheng Zhao
Adam D. Myers
Pauline Zarrouk
Jiamin Hou
Romain Paviot
Mehdi Rezaie
Jeffrey A. Newman
Ashley J. Ross
M. Vivek
Rita Tojeiro
Mariana Vargas Magaña
Brad W. Lyke
Anand Raichoor
Héctor Gil-Marín
Dmitry Bizyaev
Center for Cosmology & AstroParticle Physics
Ohio State University [Columbus] (OSU)
Institute of Cosmology and Gravitation [Portsmouth] (ICG)
University of Portsmouth
University of St Andrews [Scotland]
Institute for Astronomy [Edinburgh] (IfA)
University of Edinburgh
Lawrence Berkeley National Laboratory [Berkeley] (LBNL)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Max Planck Institute for Extraterrestrial Physics (MPE)
Max-Planck-Gesellschaft
University of Utah
Institut de Ciencies del Cosmos (ICCUB)
Universitat de Barcelona (UB)
Institute for Space Studies of Catalonia [Barcelona] (IEEC-CSIC)
Department of Physics and Astronomy [Laramie]
University of Wyoming (UW)
Department of Physics and Astronomy [Waterloo]
University of Waterloo [Waterloo]
Siena College [Loudonville]
Department of Physics [Oxford]
University of Oxford
Perimeter Institute for Theoretical Physics [Waterloo]
Ecole Polytechnique Fédérale de Lausanne (EPFL)
Ohio University - Athens (OU)
Physics & Astronomy Department [Ohio University]
Department of Physics [New York]
New York University [New York] (NYU)
NYU System (NYU)-NYU System (NYU)
National Astronomical Observatories [Beijing] (NAOC)
Chinese Academy of Sciences [Beijing] (CAS)
New Mexico State University
Centro de Investigaciones Energéticas Medioambientales y Tecnológicas [Madrid] (CIEMAT)
Sejong University
Kavli Institute for Particle Astrophysics and Cosmology (KIPAC)
Stanford University
Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM)
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Centre de Physique des Particules de Marseille (CPPM)
Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Instituto de Ciencias Físicas
Department of Physics and Astronomy [Pittsburgh]
University of Pittsburgh (PITT)
Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE)
Centro de Astronomia [Antofagasta] (CITEVA)
Universidad de Antofagasta
Center for Computational Astrophysics [New York]
Flatiron Institute
Department of Astronomy and Astrophysics [PennState]
Pennsylvania State University (Penn State)
Penn State System-Penn State System
Indian Institute of Astrophysics (IIA)
ANR-16-CE31-0021,eBOSS,Sondes cosmologiques de la gravitation et de l'énergie noire(2016)
ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011)
European Project: 670193,H2020,ERC-2014-ADG,COSFORM(2015)
University of Oxford [Oxford]
Universidad Nacional Autónoma de México (UNAM)
University of St Andrews. School of Physics and Astronomy
Alfred P. Sloan Foundation
Department of Energy (US)
European Commission
Centre National de la Recherche Scientifique (France)
National Research Foundation of Korea
Source :
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2020, 498 (2), pp.2354-2371. ⟨10.1093/mnras/staa2416⟩, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 498 (2), pp.2354-2371. ⟨10.1093/mnras/staa2416⟩, Monthly notices of the Royal Astronomical Society, 2020, Vol.498(2), pp.2354-2371 [Peer Reviewed Journal], Digital.CSIC. Repositorio Institucional del CSIC, instname
Publication Year :
2020
Publisher :
HAL CCSD, 2020.

Abstract

We present large-scale structure catalogs from the completed extended Baryon Oscillation Spectroscopic Survey (eBOSS). Derived from Sloan Digital Sky Survey (SDSS) -IV Data Release 16 (DR16), these catalogs provide the data samples, corrected for observational systematics, and random positions sampling the survey selection function. Combined, they allow large-scale clustering measurements suitable for testing cosmological models. We describe the methods used to create these catalogs for the eBOSS DR16 Luminous Red Galaxy (LRG) and Quasar samples. The quasar catalog contains 343,708 redshifts with $0.8 < z < 2.2$ over 4,808\,deg$^2$. We combine 174,816 eBOSS LRG redshifts over 4,242\,deg$^2$ in the redshift interval $0.6 < z < 1.0$ with SDSS-III BOSS LRGs in the same redshift range to produce a combined sample of 377,458 galaxy redshifts distributed over 9,493\,deg$^2$. Improved algorithms for estimating redshifts allow that 98 per cent of LRG observations result in a successful redshift, with less than one per cent catastrophic failures ($��z > 1000$ ${\rm km~s}^{-1}$). For quasars, these rates are 95 and 2 per cent (with $��z > 3000$ ${\rm km~s}^{-1}$). We apply corrections for trends between the number densities of our samples and the properties of the imaging and spectroscopic data. For example, the quasar catalog obtains a $��^2$/DoF$= 776/10$ for a null test against imaging depth before corrections and a $��^2$/DoF$=6/8$ after. The catalogs, combined with careful consideration of the details of their construction found here-in, allow companion papers to present cosmological results with negligible impact from observational systematic uncertainties.<br />Matches version accepted by MNRAS, very minor changes. A summary of all SDSS BAO and RSD measurements with accompanying legacy figures can be found here: https://www.sdss.org/science/final-bao-and-rsd-measurements/ . The full cosmological interpretation of these measurements can be found here: https://sdss.org/science/cosmology-results-from-eboss/

Details

Language :
English
ISSN :
00358711 and 13652966
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2020, 498 (2), pp.2354-2371. ⟨10.1093/mnras/staa2416⟩, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 498 (2), pp.2354-2371. ⟨10.1093/mnras/staa2416⟩, Monthly notices of the Royal Astronomical Society, 2020, Vol.498(2), pp.2354-2371 [Peer Reviewed Journal], Digital.CSIC. Repositorio Institucional del CSIC, instname
Accession number :
edsair.doi.dedup.....ea4a91f2ca96875bd19deab1de4c739d
Full Text :
https://doi.org/10.1093/mnras/staa2416⟩