The Cosmological Impact of Intrinsic Alignment Model Choice for Cosmic Shear

TL;DR

This paper examines how the choice of intrinsic alignment models affects dark energy constraints from weak lensing, emphasizing the importance of accurate IA modeling to avoid significant biases in cosmological parameters.

Contribution

It compares different IA models and demonstrates that flexible parameter grids can mitigate biases, highlighting the necessity of proper IA modeling in future surveys.

Findings

Ignoring IAs causes catastrophic bias in dark energy parameters.

Flexible IA parameter grids can recover true cosmological parameters.

The latest IA model reduces bias compared to earlier versions.

Abstract

We consider the effect of galaxy intrinsic alignments (IAs) on dark energy constraints from weak gravitational lensing. We summarise the latest version of the linear alignment model of IAs, following the brief note of Hirata & Seljak (2010) and further interpretation in Laszlo et al. (2011). We show the cosmological bias on the dark energy equation of state parameters w0 and wa that would occur if IAs were ignored. We find that w0 and wa are both catastrophically biased, by an absolute value of just greater than unity under the Fisher matrix approximation. This contrasts with a bias several times larger for the earlier IA implementation. Therefore there is no doubt that IAs must be taken into account for future Stage III experiments and beyond. We use a flexible grid of IA and galaxy bias parameters as used in previous work, and investigate what would happen if the universe used the latest IA model, but we assumed the earlier version. We find that despite the large difference between the two IA models, the grid flexibility is sufficient to remove cosmological bias and recover the correct dark energy equation of state. In an appendix, we compare observed shear power spectra to those from a popular previous implementation and explain the differences.