Fig. 11

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Best-fit values for vCDM cosmological model from eRASS1 cosmological experiment (orange), Planck CMB 2020 data (blue), and combination of eROSITA and Planck CMB (red) are shown. The SPT-SZ cluster abundances and SDSS BOSS DR16 BAO + CMB lensing results are shown in green and brown (Bocquet et al. 2019; Alam et al. 2017). SPT recent constraints from Bocquet et al. (2024) are added in purple. eRASS1 cosmological experiment places the very tight constraints on the sum of the neutrino masses to be ∑ mv < 0.43eV from cluster number counts alone.
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