4.7 Article

Intrinsic alignments in IllustrisTNG and their implications for weak lensing: Tidal shearing and tidal torquing mechanisms put to the test

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 514, Issue 2, Pages 2049-2072

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac042

Keywords

methods: numerical; galaxies: formation; cosmology: theory

Funding

  1. European Research Council (ERC) under the European Union [679145]
  2. European Research Council (ERC) [679145] Funding Source: European Research Council (ERC)

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This study tests the linear and quadratic models for intrinsic alignments by using morphologically selected samples of galaxies. The results show a significant alignment signal for elliptical galaxies, which increases with mass and redshift. On the other hand, spiral galaxies only exhibit a significant signal for the most massive objects, and the quadratic model breaks down for spiral galaxies.
Accurate measurements of the cosmic shear signal require a separation of the true weak gravitational lensing signal from intrinsic shape correlations of galaxies. These 'intrinsic alignments' of galaxies originate from galaxy formation processes and are expected to be correlated with the gravitational field through tidal processes affecting the galaxies, such as tidal shearing for elliptical galaxies and tidal torquing for spiral galaxies. In this study, we use morphologically selected samples of elliptical and spiral galaxies from the illustrisTNG simulation at z = 0 and z = 1 to test the commonly employed linear (tidal shearing) and quadratic (tidal torquing) models for intrinsic alignments. We obtain local measurements of the linear and quadratic alignment parameters, including corrections for large-scale anisotropies of the cosmologically small simulation volume, and study their dependence on galaxy and environmental properties. We find a significant alignment signal for elliptical galaxies (linear model), that increases with mass and redshift. Spiral galaxies (quadratic model), on the other hand, exhibit a significant signal only for the most massive objects at z = 1. We show the quadratic model for spiral galaxies to break down at its fundamental assumptions, and simultaneously obtain a significant signal of spiral galaxies to align according to the linear model. We use the derived alignment parameters to compute intrinsic alignment spectra and estimate the expected contamination in the weak lensing signal obtained by Euclid.

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