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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

  • Tamone, Amélie Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland
  • Raichoor, Anand Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland
  • Zhao, Cheng ORCID Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland
  • de Mattia, Arnaud IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
  • Gorgoni, Claudio Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland
  • Burtin, Etienne IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
  • Ruhlmann-Kleider, Vanina IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
  • Ross, Ashley J ORCID Center for Cosmology and AstroParticle Physics, The Ohio State University, Columbus, OH 43212, USA
  • Alam, Shadab Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
  • Percival, Will J Perimeter Institute for Theoretical Physics, 31 Caroline St. North, Waterloo, ON N2L 2Y5, Canada
  • Avila, Santiago Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
  • Chapman, Michael J Department of Physics and Astronomy, University of Waterloo, 200 University Ave W, Waterloo, ON N2L 3G1, Canada
  • Chuang, Chia-Hsun ORCID Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA
  • Comparat, Johan Max-Planck-Institut für extraterrestrische Physik (MPE), Giessenbachstrasse 1, D-85748 Garching bei München, Germany
  • Dawson, Kyle S Department of Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112, USA
  • de la Torre, Sylvain Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
  • du Mas des Bourboux, Hélion Department of Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112, USA
  • Escoffier, Stephanie Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
  • Gonzalez-Perez, Violeta ORCID Institute of Cosmology & Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX, UK
  • Hou, Jiamin Max-Planck-Institut für extraterrestrische Physik (MPE), Giessenbachstrasse 1, D-85748 Garching bei München, Germany
  • Kneib, Jean-Paul Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
  • Mohammad, Faizan G Department of Physics and Astronomy, University of Waterloo, 200 University Ave W, Waterloo, ON N2L 3G1, Canada
  • Mueller, Eva-Maria Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
  • Paviot, Romain Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
  • Rossi, Graziano Department of Physics and Astronomy, Sejong University, Seoul 143-747, Korea
  • Schneider, Donald P Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
  • Wang, Yuting National Astronomical Observatories of China, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China
  • Zhao, Gong-Bo University of Chinese Academy of Sciences, Beijing 100049, China
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  • 2020-10-5
Published in:
  • Monthly Notices of the Royal Astronomical Society. - Oxford University Press (OUP). - 2020, vol. 499, no. 4, p. 5527-5546
Space and Planetary Science
Astronomy and Astrophysics
English 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 deg2 over the redshift range 0.6 ≤ z ≤ 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, zeff = 0.85, including statistical and systematical uncertainties, we measure the linear growth rate of structure fσ8(zeff) = 0.35 ± 0.10, the Hubble distance $D_ H(z_{\rm eff})/r_{\rm drag} = 19.1^{+1.9}_{-2.1}$, and the comoving angular diameter distance DM(zeff)/rdrag = 19.9 ± 1.0. These results are in agreement with the Fourier space analysis, leading to consensus values of: fσ8(zeff) = 0.315 ± 0.095, $D_H(z_{\rm eff})/r_{\rm drag} = 19.6^{+2.2}_{-2.1}$, and DM(zeff)/rdrag = 19.5 ± 1.0, consistent with ΛCDM model predictions with Planck parameters.
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  • English
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https://sonar.ch/global/documents/282368
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