Статья

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0

Héctor Gil-MarínInstitut de Ciències del Cosmos, Universitat de Barcelona, ICCUB, Martí i Franquès 1, E-08028 Barcelona, SpainJulian BautistaInstitute of Cosmology & Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth PO1 3FX, UKRomain PaviotAix Marseille Univ, CNRS, CNES, LAM, 13013 Marseille, FranceM. Vargas-MagañaInstituto de Física, Universidad Nacional Autónoma de México, Apdo. Postal 20-364 Ciudad de México, MéxicoSylvain de la TorreAix Marseille Univ, CNRS, CNES, LAM, 13013 Marseille, FranceS. FromenteauInstituto de Ciencias Físicas, Universidad Nacional Autónoma de México, Av. Universidad s/n, 62210 Cuernavaca, Mor., MexicoShadab AlamInstitute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UKS. ÀvilaInstituto de Física Teórica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, SpainE. BurtinIRFU/CEA Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceChia-Hsun ChuangKavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USAK. S. DawsonDepartment Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112, USAJiamin HouMax-Planck-Institut für Extraterrestrische Physik, Postfach 1312, Giessenbachstr., D-85748 Garching bei München, GermanyArnaud de MattiaIRFU/CEA Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceFaizan G MohammadDepartment of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, CanadaEva-Maria MüllerUniversity of Oxford, Oxford OX1 3RH, UKS. NadathurInstitute of Cosmology & Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth PO1 3FX, UKRichard NeveuxIRFU/CEA Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceWill J. PercivalDepartment of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, CanadaAnand RaichoorInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Federale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, SwitzerlandMehdi RezaieDepartment of Physics and Astronomy, Ohio University, Clippinger Labs, Athens, OH 45701, USAA.J. RossDepartment of Physics and Astronomy, Ohio University, Clippinger Labs, Athens, OH 45701, USAGraziano RossiDepartment of Physics and Astronomy, Sejong University, Seoul 143-747, KoreaV. Ruhlmann-KleiderIRFU/CEA Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceA. G. SmithIRFU/CEA Université Paris-Saclay, F-91191 Gif-sur-Yvette, FranceAmélie TamoneInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Federale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, SwitzerlandJeremy L. TinkerCenter for Cosmology and Particle Physics, Department of Physics, New York University, New York, NY 10003, USARita TojeiroSchool of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS, UKYuting WangNational Astronomy Observatories, Chinese Academy of Science, 100012 Beijing, P.R. ChinaGong‐Bo ZhaoInstitute of Cosmology & Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth PO1 3FX, UKCheng ZhaoInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Federale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, SwitzerlandJ. BrinkmannJoel R. BrownsteinDepartment Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112, USAPeter Doohyun ChoiDepartment of Physics and Astronomy, Sejong University, Seoul 143-747, KoreaS. EscoffierAix Marseille Univ, CNRS/IN2P3, CPPM, 13288 Marseille, FranceAxel de la MacorraInstituto de Física, Universidad Nacional Autónoma de México, Apdo. Postal 20-364 Ciudad de México, MéxicoJeongin MoonDepartment of Physics and Astronomy, Sejong University, Seoul 143-747, KoreaJeffrey A. NewmanPITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USADonald P. SchneiderInstitute for Gravitation and the Cosmos, Pennsylvania State University, University Park, PA 16802, USAHee‐Jong SeoDepartment of Physics and Astronomy, Ohio University, Clippinger Labs, Athens, OH 45701, USAMariappan VivekIndian Institute of Astrophysics, Koramangala, Bangalore 560034, India

2020en

ABI

Аннотация

ABSTRACT We analyse the clustering of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey Data Release 16 luminous red galaxy sample (DR16 eBOSS LRG) in combination with the high redshift tail of the Sloan Digital Sky Survey III Baryon Oscillation Spectroscopic Survey Data Release 12 (DR12 BOSS CMASS). We measure the redshift space distortions (RSD) and also extract the longitudinal and transverse baryonic acoustic oscillation (BAO) scale from the anisotropic power spectrum signal inferred from 377 458 galaxies between redshifts 0.6 and 1.0, with the effective redshift of zeff = 0.698 and effective comoving volume of $2.72\, {\rm Gpc}^3$. After applying reconstruction, we measure the BAO scale and infer DH(zeff)/rdrag = 19.30 ± 0.56 and DM(zeff)/rdrag = 17.86 ± 0.37. When we perform an RSD analysis on the pre-reconstructed catalogue on the monopole, quadrupole, and hexadecapole we find, DH(zeff)/rdrag = 20.18 ± 0.78, DM(zeff)/rdrag = 17.49 ± 0.52 and fσ8(zeff) = 0.454 ± 0.046. We combine both sets of results along with the measurements in configuration space and report the following consensus values: DH(zeff)/rdrag = 19.77 ± 0.47, DM(zeff)/rdrag = 17.65 ± 0.30 and fσ8(zeff) = 0.473 ± 0.044, which are in full agreement with the standard ΛCDM and GR predictions. These results represent the most precise measurements within the redshift range 0.6 ≤ z ≤ 1.0 and are the culmination of more than 8 yr of SDSS observations.

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Идентификаторы

DOI: 10.1093/mnras/staa2455

Цитирования и источники

Цитирований: 10Использованных источников: 0

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