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Table 1.

Summary of the best-fit parameters (see Eqs. (1)–(3)) and derived quantities (luminosity values) obtained from fitting the three forward models from this work to the Fullphot X-ray surface brightness profile.

Best-fit 𝒩sat fsat Best-fit 𝒩ps LX,  PS LX,  cenCGM χred2
[10 34 ergs s kpc 2 $ ^{34}\,\frac{\mathrm{ergs}}{\mathrm{s\,kpc^2}} $] ergs s kpc 2 $ \frac{\mathrm{ergs}}{\mathrm{s\,kpc^2}} $ [ergs/s] [ergs/s]
Model 1 2 . 75 0.12 + 0.12 $ 2.75_{-0.12}^{+0.12} $ 0.31 7 . 6 1.6 + 2.2 × 10 36 $ 7.6_{-1.6}^{+2.2}\times 10^{36} $ 7 . 851 0.274 + 0.028 × 10 39 $ 7.851_{-0.274}^{+0.028}\times 10^{39} $ 6 . 58 0.94 + 0.27 × 10 40 $ 6.58_{-0.94}^{+0.27}\times 10^{40} $ 0.44
Model 2 2 . 95 0.13 + 0.14 $ 2.95_{-0.13}^{+0.14} $ 0.33 1 . 1 0.2 + 0.2 × 10 37 $ 1.1_{-0.2}^{+0.2}\times 10^{37} $ 1 . 195 0.042 + 0.003 × 10 40 $ 1.195_{-0.042}^{+0.003}\times 10^{40} $ 2 . 76 0.19 + 0.06 × 10 40 $ 2.76_{-0.19}^{+0.06}\times 10^{40} $ 1.32
Model 3 1 . 51 0.073 + 0.07 $ 1.51_{-0.073}^{+0.07} $ 0.56 1 . 5 0.2 + 0.2 × 10 37 $ 1.5_{-0.2}^{+0.2}\times 10^{37} $ 1 . 576 0.063 + 0.001 × 10 40 $ 1.576_{-0.063}^{+0.001}\times 10^{40} $ 1 . 69 0.91 + 0.28 × 10 40 $ 1.69_{-0.91}^{+0.28}\times 10^{40} $ 1.89

Notes. For every model, we present the best-fit 𝒩sat: renormalization of the SX,  sat (of the TNG300-based prediction), fsat: the fraction of satellites in the mock galaxy catalog (see descriptions of the mock catalogs in Sect. 3.3), 𝒩ps: the normalization of the point-source component (see Eq. (2)), LX,  PS: the X-ray luminosity obtained by integrating the point source component, LX,  cenCGM: the X-ray luminosity obtained by integrating the central galaxies hot CGM component, χred2: the reduced χ2 statistic for the model, obtained by using 21 − 2 degrees of freedom.

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