A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
Daniel Martens, Christopher M. Hirata, Ashley J. Ross, Xiao Fang

TL;DR
This paper measures galaxy radial intrinsic alignments using BOSS data, providing evidence for their existence and consistency with theoretical models, which impacts cosmological analyses involving galaxy clustering anisotropies.
Contribution
It introduces a novel measurement of radial galaxy alignments using orientation-dependent selection effects in BOSS data, testing theoretical predictions.
Findings
Measured alignment parameter B for CMASS and LOWZ samples.
Found the ratio of observed to theoretical alignment values around 0.6.
Provided evidence (2-3 sigma) for radial intrinsic galaxy alignments.
Abstract
The anisotropy of galaxy clustering in redshift space has long been used to probe the rate of growth of cosmological perturbations. However, if galaxies are aligned by large-scale tidal fields, then a sample with an orientation-dependent selection effect has an additional anisotropy imprinted onto its correlation function. We use the LOWZ and CMASS catalogs of SDSS-III BOSS Data Release 12 to divide galaxies into two sub-samples based on their offset from the Fundamental Plane, which should be correlated with orientation. These sub-samples must trace the same underlying cosmology, but have opposite orientation-dependent selection effects. We measure the clustering parameters of each sub-sample and compare them in order to calculate the dimensionless parameter , a measure of how strongly galaxies are aligned by gravitational tidal fields. We found that for CMASS (LOWZ), the measured…
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