Fig. 17.
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Best fit of a linear model to the RLF of the MaDCoWS clusters determined using NVSS 1.4 GHz fluxes (Sect. 5.3) vs. richness. The best fit is inconsistent with the null hypothesis of no evolution of the RLF with richness at 5.9σ. In comparison to Mo et al. (2020), we favor a higher slope for the relation at 1.2σ, although see the discussion in Sect. 7.1.2.
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