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Table 1.

Fiducial cosmological parameters.

S8 Ωm Ωb h ns AIA Abary
0.759 0.246 0.015 0.767 0.901 0.264 2.859

Notes. We employ a flat ΛCDM model with parameters fitted to the KiDS-1000 cosmic shear data (Asgari et al. 2021). The structure growth parameter, S8 = σ8m/0.3)0.5, and the amplitude of the intrinsic alignments of galaxies, AIA, are the only two parameters that KiDS-1000 cosmic shear data constrain. Ωm is the total matter density parameter, and Ωb represents the density parameter for baryonic matter. The spectral index of the primordial power spectrum is denoted as ns, while h represents the dimensionless Hubble parameter. We allow for baryonic feedback through Abary, which is equal to 3.13 for a dark-matter-only scenario. Additionally, the sum of the neutrino masses is fixed to 0.06 eV.

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