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Table A.1.

Summary of the regression analysis for the redshift z > 0.06 sample a

Sample Intercept α Slope β Intrinsic scatter σ N clusters Figure
Compact D10 vs. σv 1.203 ± 0.158 2.357 ± 0.392 0.299 ± 0.053 339 A.1 & A.2
Extended D10 vs. σv 1.429 ± 0.187 1.878 ± 0.387 0.284 ± 0.052 175 A.1 & A.2
Compact LX vs. σv 98.405 ± 0.368 5.354 ± 0.852 0.392 ± 0.121 339 A.3 & A.4
Extended LX vs. σv 98.987 ± 0.424 4.536 ± 0.855 0.479 ± 0.121 175 A.3 & A.4
Compact D10 vs. LX 1.656 ± 0.071 0.303 ± 0.041 0.418 ± 0.026 339 A.5 & A.6
Extended D10 vs. LX 1.634 ± 0.100 0.313 ± 0.044 0.333 ± 0.029 175 A.5 & A.6
Compact LX vs. σvD10 < 9. 98.588 ± 0.884 5.764 ± 5.033 0.321 ± 0.242 192 A.7 & A.8
Extended LX vs. σvD10 < 9. 99.444 ± 0.936 2.815 ± 4.513 0.469 ± 0.361 70 A.7 & A.8
Compact LX vs. σvD10 > 9. 98.317 ± 0.505 5.500 ± 1.126 0.413 ± 0.134 147 A.7 & A.8
Extended LX vs. σvD10 > 9. 98.937 ± 0.502 4.636 ± 1.011 0.475 ± 0.133 105 A.7 & A.8

a On the X-axis: LX has been normalized by 1043 erg s−1, σv by 400 km s−1. To account for the evolution of the scaling relations, we use LXEz−1.

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