Fig. 3.

Top panels: global properties (empty black dots) and after correction for the Ez factor (solid red dots) recovered from their thermodynamic profiles for the following input values for (M500, z): (8 × 1014 M⊙, 0.05), (5 × 1014 M⊙, 0.05), (2 × 1014 M⊙, 0.05), (8 × 1014 M⊙, 0.5), (5 × 1014 M⊙, 0.5), (2 × 1014 M⊙, 1). The dashed magenta lines identify the best-fit relations of Eq. (7). A core-excised bolometric luminosity is considered. Bottom panels: red dots are the quantities (from left to right: fg, fT, b) estimated in our model for the following input values for (M500, z): (8 × 1014 M⊙, 0.05), (5 × 1014 M⊙, 0.05), (2 × 1014 M⊙, 0.05), (8 × 1014 M⊙, 0.5), (5 × 1014 M⊙, 0.5), and (2 × 1014 M⊙, 1); the blue dotted line indicates Ωb/Ωm = 0.157 (Planck Collaboration XXVII 2016); the dashed magenta lines show the predictions following the relations: fg = 0.124 𝒯0.23, fT = 0.687 𝒯0.07 and 1 − b = h0 = 1, where fg and fT are the absolute values, i.e. multiplied by the assumed normalisations of 0.1 and , respectively.
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