Notes. Here, 𝒰 stands for a uniform prior and 𝒩(μ, σ²) for a Gaussian prior with mean μ and variance σ². The cosmological parameters are listed in the top subpanel and the non-cosmological parameters are listed in the bottom subpanel. For the stochastic parameters, the prior width on sn₀ is scaled by the Poissonian shot-noise ($1/{\overline{n}}_g$), while the prior widths for sn₂ and sn₄ are scaled by the expected fraction of satellite galaxies, the effective velocity dispersion of the satellites, and the Poissonian shot-noise: $f_{\mathrm{sat}}{\sigma }_{1\mathrm{eff}}^2/{\overline{n}}_g$, $f_{\mathrm{sat}}{\sigma }_{1\mathrm{eff}}^4/{\overline{n}}_g$, respectively (see Maus et al. (2024) for details).