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Fig. B.4
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Posterior on Ωm-σ8 from the ΛCDM, vCDM, wCDM, vwCDM, and ΛCDM with ∑ mv = 0.06 eV fits from our eRASS1 cluster dataset. We see the nice overlap in the parameter space that indicates that our fit in the Ωm-σ8 plane is stable against modification to the standard ΛCDM cosmological model.
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