All Tables

Table 1: General cluster properties. Column (1): cluster name; Col. (2): right ascension; Col. (3): declination; Col. (4): redshift; Col. (5): luminosity distance; Col. (6): hydrogen column density (Dickey & Lockman 1990); Col. (7): X-ray emission mean temperature derived in this work; see Sect. 4.2; Col. (8): r₅₀₀ values were derived in this work.
Table 2: Observational information of the XMM-Newton data. Column (1): cluster name; Col. (2): filter in which cluster was observed; Col. (3): total exposure time; Cols. (4-6): exposure time after flare cleaning in each detector.
Table 3: Fits results. Column (1): cluster name; Col. (2): slope parameter of the $\beta$ -model; Cols. (3, 4): scale radius in arcsec and in $h_{\rm 70}^{-1}$ kpc of the $\beta$ -model; Col. (5): electron number density of the central region calculated by means of the $\beta$ -model; Col. (6): slope parameter of the Sérsic fit; Cols. (7, 8) scale radius in arcsec and in $h_{\rm 70}^{-1}$ kpc of the Sérsic model; Col. 9 electron number density of the central region calculated by means of the Sérsic model.
Table 4: Best fit results for the parameters of 2D temperature profiles (Eq. (9)) for A496, A1689 and A2667.
Table 5: Luminosity function fits results. For A496 we present the results for single and double Schechter fits.
Table 6: Gas and total mass determination from X-ray data. Column (1): cluster name; Cols. (2, 3): gas and total mass calculated by means of the $\beta$ -model; Cols. (4, 5): gas and total mass calculated by means of the Sérsic model; Col. (6): gas fraction ( $M_{\rm {gas}}/M_{\rm {tot}}$ ) calculated by means of the best model. Values in bold represent the best model for the cluster.
Table 7: Results derived from optical data. Column (1): cluster name; Col. (2): total luminosity derived from stars within galaxies; Col. (3): fraction of star forming galaxies; Col. (4): stellar mass; Col. (5): ICL mass; Col. (6): stellar and ICL mass to gas mass fraction.