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Table 7.

Best linear fit parameters for ln(SFR/Myr−1) vs. ln(dsep/R200) relationships for BGGs in different subsamples (S-I to S-V).

Sample Subsample α β σ
S-I COSMOS −1.972 ± 0.356 −0.114 ± 0.145 1.538 ± 0.171
H15 0.012 ± 0.085 0.118 ± 0.011 2.162 ± 0.032
Magneticum −2.088 ± 0.469 −0.508 ± 0.153 1.682 ± 0.067
S-II COSMOS −2.613 ± 0.726 −0.300 ± 0.220 1.775 ± 0.329
H15 −0.065 ± 0.156 0.090 ± 0.023 2.028 ± 0.066
Magneticum 1.258 ± 0.445 −0.149 ± 0.134 1.579 ± 0.067
S-III COSMOS −0.475 ± 0.706 −0.034 ± 0.435 1.910 ± 0.318
H15 0.684 ± 0.067 0.129 ± 0.009 1.911 ± 0.025
Magneticum 1.482 ± 0.168 −0.241 ± 0.050 1.458 ± 0.029
S-IV COSMOS 0.299 ± 0.785 0.415 ± 0.392 2.524 ± 0.338
H15 1.292 ± 0.290 0.803 ± 0.036 6.103 ± 0.078
Magneticum 2.564 ± 0.207 −0.150 ± 0.062 1.189 ± 0.035
S-V COSMOS 0.632 ± 0.915 −0.136 ± 0.482 3.214 ± 0.503
H15 2.142 ± 0.122 0.155 ± 0.015 1.875 ± 0.038
Magneticum 2.988 ± 0.281 −0.314 ± 0.082 0.854 ± 0.057
combined (S-I to S-V) COSMOS −0.451 ± 0.261 0.077 ± 0.112 2.321 ± 0.122
H15 0.790 ± 0.034 0.113 ± 0.004 2.108 ± 0.012
Magneticum −0.342 ± 0.082 −0.458 ± 0.027 1.942 ± 0.014

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