Table 4
Comparison of the cluster galaxy population VDPs.
| Stack | Classes | Prob | VDP ratio y/x | |
| x vs. y | ≤ 0.5r200 | > 0.5r200 | ||
|
|
||||
| Reg-sigv | E vs. S0 | 0.184 | 1.08 ± 0.08 | 1.04 ± 0.09 |
| E vs. S | < 0.001 | 1.27 ± 0.11 | 1.22 ± 0.06 | |
| S0 vs. S | < 0.001 | 1.17 ± 0.04 | 1.17 ± 0.04 | |
| Irr-sigv | E vs. S0 | 0.125 | 1.15 ± 0.07 | 0.98 ± 0.10 |
| E vs. S | 0.010 | 1.35 ± 0.07 | 1.03 ± 0.04 | |
| S0 vs. S | 0.194 | 1.08 ± 0.10 | 1.06 ± 0.11 | |
| Reg-Num | E vs. S0 | 0.287 | 1.04 ± 0.08 | 0.96 ± 0.04 |
| E vs. S | < 0.001 | 1.24 ± 0.06 | 1.12 ± 0.02 | |
| S0 vs. S | 0.008 | 1.11 ± 0.00 | 1.09 ± 0.04 | |
| Irr-Num | E vs. S0 | 0.084 | 1.15 ± 0.11 | 0.94 ± 0.09 |
| E vs. S | 0.017 | 1.26 ± 0.05 | 0.94 ± 0.02 | |
| S0 vs. S | 0.150 | 1.12 ± 0.07 | 0.91 ± 0.15 | |
Notes. “Prob” indicates the probability that the VDPs of the x and y populations are the same. We consider probabilities <0.05 as indicating a significant difference in the VDPs. These cases are highlighted in boldface in the table. The VDP ratios are computed in two radial bins.
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