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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

Authors :
Gil-Marín, Héctor
Bautista, Julián E.
Paviot, Romain
Vargas-Magaña, Mariana
de la Torre, Sylvain
Fromenteau, Sebastien
Alam, Shadab
Ávila, Santiago
Burtin, Etienne
Chuang, Chia-Hsun
Dawson, Kyle S.
Hou, Jiamin
de Mattia, Arnaud
Mohammad, Faizan G.
Müller, Eva-Maria
Nadathur, Seshadri
Neveux, Richard
Percival, Will J.
Raichoor, Anand
Rezaie, Mehdi
Ross, Ashley J.
Rossi, Graziano
Ruhlmann-Kleider, Vanina
Smith, Alex
Tamone, Amélie
Tinker, Jeremy L.
Tojeiro, Rita
Wang, Yuting
Zhao, Gong-Bo
Zhao, Cheng
Brinkmann, Jonathan
Brownstein, Joel R.
Choi, Peter D.
Escoffier, Stephanie
de la Macorra, Axel
Moon, Jeongin
Newman, Jeffrey A.
Schneider, Donald P.
Seo, Hee-Jong
Vivek, Mariappan
Source :
Monthly Notices of the Royal Astronomical Society 2020, Volume 498, Issue 2, pp.2492-2531
Publication Year :
2020

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 effective redshift of $z_{\rm eff}=0.698$ and effective comoving volume of $2.72\,{\rm Gpc}^3$. After applying reconstruction we measure the BAO scale and infer $D_H(z_{\rm eff})/r_{\rm drag} = 19.30\pm 0.56$ and $D_M(z_{\rm eff})/r_{\rm drag} =17.86 \pm 0.37$. When we perform a redshift space distortions analysis on the pre-reconstructed catalogue on the monopole, quadrupole and hexadecapole we find, $D_H(z_{\rm eff})/r_{\rm drag} = 20.18\pm 0.78$, $D_M(z_{\rm eff})/r_{\rm drag} =17.49 \pm 0.52$ and $f\sigma_8(z_{\rm eff})=0.454\pm0.046$. We combine both sets of results along with the measurements in configuration space of \cite{LRG_corr} and report the following consensus values: $D_H(z_{\rm eff})/r_{\rm drag} = 19.77\pm 0.47$, $D_M(z_{\rm eff})/r_{\rm drag} = 17.65\pm 0.30$ and $f\sigma_8(z_{\rm eff})=0.473\pm 0.044$, which are in full agreement with the standard $\Lambda$CDM and GR predictions. These results represent the most precise measurements within the redshift range $0.6\leq z \leq 1.0$ and are the culmination of more than 8 years of SDSS observations.<br />Comment: 41 pages, 20 figures; Minor updates to match the published version in MNRAS. 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

Database :
arXiv
Journal :
Monthly Notices of the Royal Astronomical Society 2020, Volume 498, Issue 2, pp.2492-2531
Publication Type :
Report
Accession number :
edsarx.2007.08994
Document Type :
Working Paper
Full Text :
https://doi.org/10.1093/mnras/staa2455