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Table 4

Best-fit results of the spectral and spatial analysis of the sample of galaxy clusters at an overdensity corresponding to 4500.

β-model metal maps
Cluster k Tgas Z/Z rc β Δ Mtot Mgas Mmetals Mmetals Ratio
 keV kpc 1013   M 1012   M 1010   M 1010   M C. 10 to C. 9

Sérsic 2.38  ±  0.01 0.357  ±  0.003 37  ±  1 0.602  ±  0.001 4500 2.59  ±  0.18 2.45  ±  0.12 1.75  ±  0.09 1.92  ±  0.25 1.34  ±  0.23
Centaurus 3.74  ±  0.01 0.810  ±  0.003 17  ±  1 0.397  ±  0.001 4500 2.91  ±  0.14 1.20  ±  0.11 1.94  ±  0.19 2.17  ±  0.18 1.12  ±  0.19
Hydra 3.57  ±  0.01 0.357  ±  0.005 35  ±  1 0.561  ±  0.001 4500 3.76  ±  0.22 3.36  ±  0.20 2.40  ±  0.14 3.32  ±  0.59 1.38  ±  0.31
A496 3.72  ±  0.01 0.586  ±  0.004 27  ±  1 0.459  ±  0.001 4500 3.76  ±  0.19 2.72  ±  0.16 3.19  ±  0.18 3.91  ±  0.45 1.23  ±  0.20
A2029 7.01  ±  0.02 0.493  ±  0.006 41  ±  1 0.563  ±  0.001 4500 12.26  ±  0.81 11.42  ±  0.83 11.79  ±  1.01 13.97  ±  0.95 1.18  ±  0.16

Sérsic 2.39  ±  0.01 0.309  ±  0.003 37  ±  1 0.602  ±  0.001 2500 3.95  ±  0.11 3.95  ±  0.21 2.44  ±  0.13 3.03  ±  0.21 1.24 ± 0.19
Hydra 3.46  ±  0.01 0.346  ±  0.005 35  ±  1 0.561  ±  0.001 2500 5.47  ±  0.29 5.53  ±  0.41 3.83  ±  0.43 4.97  ±  0.55 1.30  ±  0.26
A496 3.80  ±  0.01 0.506  ±  0.004 27  ±  1 0.459  ±  0.001 2500 5.30  ±  0.20 4.79  ±  0.31 4.85  ±  0.31 6.38  ±  0.70 1.32  ±  0.22
A2029 7.07  ±  0.02 0.468  ±  0.006 41  ±  1 0.563  ±  0.001 2500 17.5  ±  0.90 21.8  ±  1.30 20.4  ±  1.20 23.7  ±  2.80 1.16  ±  0.19

A496 4.43  ±  0.01 0.486  ±  0.004 27  ±  1 0.459  ±  0.001 1600 7.78  ±  0.36 6.79  ±  0.33 6.60  ±  0.38 8.79  ±  1.00 1.33  ±  0.21
Hydra 3.64  ±  0.01 0.299  ±  0.005 35  ±  1 0.561  ±  0.001 1400 8.35  ±  0.44 10.29  ±  0.56 6.15  ±  0.34 7.63  ±  0.99 1.24  ±  0.22
Sérsic 2.31  ±  0.01 0.286  ±  0.003 37  ±  1 0.602  ±  0.001 1200 5.05  ±  0.34 6.79  ±  0.29 3.88  ±  0.29 4.83  ±  0.32 1.24  ±  0.16
A2029 7.81  ±  0.02 0.420  ±  0.005 41  ±  1 0.563  ±  0.001 1200 34.0  ±  1.80 25.3  ±  1.30 21.3  ±  1.04 49.3  ±  9.90 2.31  ±  0.55

Notes. We determined the total mass using the T derived fitting the spectra with a single temperature model. The last column represents the ratio between columns 10 and 9 containing the metal mass.

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