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The completed SDSS-IV extended baryon oscillation spectroscopic survey: growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the emission-line galaxy sample

Authors :
Santiago Avila
Yuting Wang
Violeta Gonzalez-Perez
Arnaud de Mattia
Kyle S. Dawson
Shadab Alam
Gong-Bo Zhao
Will J. Percival
Anand Raichoor
Romain Paviot
Claudio Gorgoni
Jiamin Hou
Faizan G. Mohammad
Cheng Zhao
Eva Maria Mueller
Ashley J. Ross
Graziano Rossi
Jean-Paul Kneib
V. Ruhlmann-Kleider
Hélion du Mas des Bourboux
Amélie Tamone
Sylvain de la Torre
Etienne Burtin
Stephanie Escoffier
Donald P. Schneider
Chia-Hsun Chuang
Johan Comparat
Michael J. Chapman
Ecole Polytechnique Fédérale de Lausanne (EPFL)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Center for Cosmology & AstroParticle Physics
Ohio State University [Columbus] (OSU)
Institute for Astronomy [Edinburgh] (IfA)
University of Edinburgh
Perimeter Institute for Theoretical Physics [Waterloo]
Department of Physics and Astronomy [Waterloo]
University of Waterloo [Waterloo]
Universidad Autonoma de Madrid (UAM)
Instituto de Física Teórica UAM/CSIC (IFT)
Universidad Autonoma de Madrid (UAM)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)
Kavli Institute for Particle Astrophysics and Cosmology (KIPAC)
Stanford University
Max-Planck-Institut für Extraterrestrische Physik (MPE)
University of Utah
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)
Institute of Cosmology and Gravitation [Portsmouth] (ICG)
University of Portsmouth
Astrophysics Research Institute [Liverpool] (ARI)
Liverpool John Moores University (LJMU)
Max Planck Institute for Extraterrestrial Physics (MPE)
Max-Planck-Gesellschaft
Department of Physics [Oxford]
University of Oxford [Oxford]
Sejong University
Institute for Gravitation and the Cosmos [PennState]
Pennsylvania State University (Penn State)
Penn State System-Penn State System
Chinese Academy of Sciences [Beijing] (CAS)
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)
European Project: 290975,EC:FP7:ERC,ERC-2011-ADG_20110209,LIDA(2012)
Universidad Autónoma de Madrid (UAM)
Universidad Autónoma de Madrid (UAM)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)
University of Oxford
Source :
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩, Monthly Notices of the Royal Astronomical Society, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩
Publisher :
OXFORD UNIV PRESS

Abstract

We present the anisotropic clustering of emission line galaxies (ELGs) from the Sloan Digital Sky Survey IV (SDSS-IV) extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 16 (DR16). Our sample is composed of 173,736 ELGs covering an area of 1170 deg$^2$ over the redshift range $0.6 \leq z \leq 1.1$. We use the Convolution Lagrangian Perturbation Theory in addition to the Gaussian Streaming Redshift-Space Distortions to model the Legendre multipoles of the anisotropic correlation function. We show that the eBOSS ELG correlation function measurement is affected by the contribution of a radial integral constraint that needs to be modelled to avoid biased results. To mitigate the effect from unknown angular systematics, we adopt a modified correlation function estimator that cancels out the angular modes from the clustering. At the effective redshift, $z_{\rm eff}=0.85$, including statistical and systematical uncertainties, we measure the linear growth rate of structure $f\sigma_8(z_{\rm eff}) = 0.35\pm0.10$, the Hubble distance $D_H(z_{\rm eff})/r_{\rm drag} = 19.1^{+1.9}_{-2.1}$ and the comoving angular diameter distance $D_M(z_{\rm eff})/r_{\rm drag} = 19.9\pm1.0$. These results are in agreement with the Fourier space analysis, leading to consensus values of: $f\sigma_8(z_{\rm eff}) = 0.315\pm0.095$, $D_H(z_{\rm eff})/r_{\rm drag} = 19.6^{+2.2}_{-2.1}$ and $D_M(z_{\rm eff})/r_{\rm drag} = 19.5\pm1.0$, consistent with $\Lambda$CDM model predictions with Planck parameters.<br />Comment: 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://www.sdss.org/science/cosmology-results-from-eboss/

Details

ISSN :
00358711 and 13652966
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩, Monthly Notices of the Royal Astronomical Society, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩
Accession number :
edsair.doi.dedup.....4247d935c467eee5fdce457daaddf5ec
Full Text :
https://doi.org/10.1093/mnras/staa3050⟩