Fig. 7.
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Contour plot of the two-dimensional posterior distribution of ΩM and σ8 for the three MCMC runs where the astrophysical and cosmological parameters are jointly analysed, namely within ΛCDM (in green), within ω0CDM (in red), and within ω0ωaCDM (in blue). Moreover, in order to compare with previous results, those by Bonavera et al. (2020) are shown in black. The contours are set to 0.393 and 0.865.
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