Published best-fitting cosmological parameters for the surveys (KiDS-450, CFHTLenS, and DES-SV: Hildebrandt et al. 2017; Heymans et al. 2013; Abbott et al. 2016), and the simulation (SLICS, Harnois-Déraps et al. 2018), that we use in this paper.
Notes. σ8 is the standard deviation of perturbations in a sphere of radius 8 h−1 Mpc today. ns is the spectral index of the primordial power spectrum. Ωm and Ωb are the matter and baryon density parameters, respectively and h is the dimensionless Hubble parameter. The underlying cosmology for all cases is a flat ΛCDM model with Gaussian initial perturbations. The final column shows AIA, the amplitude of the intrinsic galaxy alignment model. DES-SV best-fit parameters are provided by Zuntz (2018, priv. comm.).
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