Fig. 6.
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One-dimensional posterior distributions of ΩM, σ8, and h (from left to right) for the results in Bonavera et al. (2020) (black solid lines), and for the three MCMC runs performed jointly on the astrophysical and cosmological parameter in this work, namely within ΛCDM (red dashed lines), within ω0CDM (blue dotted lines), and within ω0ωaCDM (green dash-dotted lines).
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