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
H\'ector Gil-Mar\'in, Juli\'an E. Bautista, Romain Paviot, Mariana, Vargas-Maga\~na, Sylvain de la Torre, Sebastien Fromenteau, Shadab Alam,, Santiago \'Avila, Etienne Burtin, Chia-Hsun Chuang, Kyle S. Dawson, Jiamin, Hou, Arnaud de Mattia, Faizan G. Mohammad, Eva-Maria M\"uller

TL;DR
This paper presents precise measurements of BAO and growth rate of structure from SDSS data between redshifts 0.6 and 1.0, confirming standard cosmological models with high accuracy.
Contribution
The study provides the most precise BAO and RSD measurements in the redshift range 0.6 to 1.0, combining multiple data sets and analysis methods for robust cosmological constraints.
Findings
Measured BAO scale with high precision at $z_{eff}=0.698$
Derived growth rate $f\sigma_8$ consistent with $\\Lambda$CDM
Results agree with standard cosmological predictions
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 and effective comoving volume of . After applying reconstruction we measure the BAO scale and infer and . When we perform a redshift space distortions analysis on the…
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