Fig. 17

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Uncertainties of the eRASS1 photometric cluster redshifts. The black dots are the formal uncertainties calculated by eROMaPPer as the standard deviation of the redshift posterior P(z). We adopted them as the final redshift uncertainties zλ,err. The dashed red line is the mean of the upper and lower empirical uncertainties
derived from the comparison to the spectroscopic cluster redshifts. The continuous red line is the absolute redshift bias |Δzλ|.
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