Fig. 8.
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Upper panel: Comparison of the observed Ygas versus mass relations within R500 with the fgas values within the same radius as given by Bulbul et al. (2024) for the eRASS:1 extended objects at z < 0.05 and with an optical counterpart. Lower panel: Residuals of the eRASS:1 data from the best fit of Fig. 4 expressed in dex (log(fgas)−log(fit)).
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