KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing

Open Access

Fig. A.3.

Posterior PDF of f_δ, mn at $k = 1.8 h {Mpc}^{- 1}$ $k = 1.8\,h\,\rm Mpc^{-1}$ in three separate redshift bins Z₁ = [0, 0.3], Z₂ = [0.3, 0.5], and Z₃ = [0.6, 2]. The filled regions are PDFs for a noisy verification run with f_δ(k, z)≡1, as in Fig. A.2, and the lines use the KiDS-1000 tomographic data (without marginalisation of projection parameters).

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