Fig. 6.
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Constraints obtained on the power spectrum reduction model from eRASS1 cluster counts combined with the sound horizon priors from the CMB Planck20. These are compared with the prediction from Lin et al. (2024) when the authors used DES-Y3 data to constrain the model. The two surveys are in agreement, although eRASS1 data points to a reduction of structure formation at low redshift.
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