Broadband Alcock-Paczynski test exploiting redshift distortions
Yong-Seon Song, Teppei Okumura, Atsushi Taruya

TL;DR
This paper introduces a broadband Alcock-Paczynski method utilizing redshift distortions and BAO features to precisely measure cosmological distances, demonstrating its effectiveness with mock catalogues.
Contribution
It presents a novel broadband AP test based on the shape of the 2D BAO circle, improving distance measurements by accounting for redshift distortions and galaxy bias.
Findings
Achieved several percent fractional errors in distance measurements.
Successfully matched coherent motion with fiducial values.
Validated the method using BOSS-like mock catalogues.
Abstract
Baryon acoustic oscillations (BAO), known as one of the largest cosmological objects, is now recognized as standard cosmological tool to measure geometric distances via the Alcock-Paczynski effect, by which the observed BAO exhibits characteristic anisotropies in addition to the redshift distortions. This implies that once we know the correct distances to the observed BAO, the tip points of baryon acoustic peaks in the anisotropic correlation function of galaxies, , can form a great circle (hereafter 2D BAO circle) in the and plane, where and are the separation of galaxy pair parallel and perpendicular to the line-of-sight, respectively. This 2D BAO circle remains unchanged under the variations of the unknown galaxy bias and/or coherent motion, while it varies transversely and radially with respect to the variations of and ,…
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