Cosmological Information in the Intrinsic Alignments of Luminous Red Galaxies
Nora Elisa Chisari (1), Cora Dvorkin (2) ((1) Princeton University,, (2) Institute for Advanced Study, Princeton)

TL;DR
This paper investigates how intrinsic galaxy alignments, especially of luminous red galaxies, encode cosmological information like BAO and primordial non-Gaussianity, using forecasts for current and future spectroscopic surveys.
Contribution
It provides the first detailed forecasts of the cosmological information in intrinsic alignments for upcoming galaxy surveys, focusing on BAO and non-Gaussianity constraints.
Findings
BAO signal in intrinsic alignments is marginally detectable in current surveys.
Future surveys like DESI and EUCLID will significantly improve BAO detection in alignments.
Primordial non-Gaussianity signals are weak and marginally detectable in intrinsic alignments.
Abstract
The intrinsic alignments of galaxies are usually regarded as a contaminant to weak gravitational lensing observables. The alignment of Luminous Red Galaxies, detected unambiguously in observations from the Sloan Digital Sky Survey, can be reproduced by the linear tidal alignment model of Catelan, Kamionkowski & Blandford (2001) on large scales. In this work, we explore the cosmological information encoded in the intrinsic alignments of red galaxies. We make forecasts for the ability of current and future spectroscopic surveys to constrain local primordial non-Gaussianity and Baryon Acoustic Oscillations (BAO) in the cross-correlation function of intrinsic alignments and the galaxy density field. For the Baryon Oscillation Spectroscopic Survey, we find that the BAO signal in the intrinsic alignments is marginally significant with a signal-to-noise ratio of 1.8 and 2.2 with the current…
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