The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the Quasar sample between redshift 0.8 and 2.2
Richard Neveux (1), Etienne Burtin (1), Arnaud de Mattia (1), Alex, Smith (1), Ashley J. Ross (2), Jiamin Hou (3), Julian Bautista (4), Jonathan, Brinkmann (5), Chia-Hsun Chuang (6), Kyle S. Dawson (7), H\'ector Gil-Mar\'in, (8, 9), Brad W. Lyke (10), Axel de la Macorra (11)

TL;DR
This paper presents BAO and RSD measurements from the anisotropic power spectrum of quasars in the eBOSS DR16, providing constraints on cosmological distances and growth rate at redshift 1.48, consistent with Planck cosmology.
Contribution
First detailed anisotropic power spectrum analysis of quasars in eBOSS DR16, including systematic error treatment and combined BAO and RSD constraints.
Findings
Measured $D_M/r_{drag}$ and $D_H/r_{drag}$ with ~3% precision.
Constrained growth rate $f(z)\sigma_8(z)$ at redshift 1.48.
Results agree with Planck $ m extLambda$CDM model.
Abstract
We measure the clustering of quasars of the final data release (DR16) of eBOSS. The sample contains quasars between redshifts over . We calculate the Legendre multipoles (0,2,4) of the anisotropic power spectrum and perform a BAO and a Full-Shape (FS) analysis at the effective redshift . The errors include systematic errors that amount to 1/3 of the statistical error. The systematic errors comprise a modelling part studied using a blind N-Body mock challenge and observational effects studied with approximate mocks to account for various types of redshift smearing and fibre collisions. For the BAO analysis, we measure the transverse comoving distance and the Hubble distance . This agrees with the configuration space…
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