Table B.1.
Correlation properties of the u − i color and the trps with the cluster-centric distance for the sample of high-spin galaxies.
| Linear fit | Spearman correlation | |||
|---|---|---|---|---|
| Relation | Slope | Intercept | ρ | Probability |
| (1) | (2) | (3) | (4) | (5) |
| u − i vs DM87 | −0.19 ± 0.07 mag Mpc−1 | 1.82 ± 0.07 mag | -0.28 | 98.2% |
| trps vs DM87 | 0.52 ± 0.23 Gyr Mpc−1 | 11.82 ± 0.23 Gyr | 0.29 | 99.0% |
Notes. (1) Correlating quantities; (2) Slope of the linear regression fit using linmix; (3) Intercept of the linear regression fit; (4) Spearman correlation coefficient for the sample; (5) Probability that the two variables are correlated.
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