Extended marginalised 1D and 2D posteriors for relevant ΛCDM and astrophysical parameters: the matter density parameter (Ω_m), the amplitude of matter density fluctuations (), σ₈ as a derived parameter, the physical baryonic matter density (Ω_bh²), the dimensionless Hubble constant (h), and the spectral index (n_s). Included are also two nuisance parameters: the amplitude of intrinsic alignments (A_IA) and the baryonic feedback amplitude (A_bary) as these correlate with some cosmological parameters. When combining the KiDS-1000 pseudo-C_ℓ constraints (red) with the SDSS BAO and RSD constraints (blue), we obtain constraints (purple) that break a few degeneracies that cosmic shear alone cannot. For comparison, we added the Planck 2018 TTTEEE-lowE (Planck Collaboration V 2020) constrains (green) and the KiDS-1000 band-powers constraints (orange) from Asgari et al. (2021).