Table 1
Spearman rank correlation parameters.
| [OIII] | Hα | stars | |
| ρ (p-value) | ρ (p-value) | ρ (p-value) | |
|
|
|||
| σ vs. SFR | 0.906 (1.5E-19) | 0.918 (7.5E-21) | 0.795 (5.4E-12) |
| v15.9 vs. SFR | 0.826 (1.6E-13) | 0.852 (4.4E-15) | 0.825 (1.7E-13) |
| v2.3 vs. SFR | 0.891 (4.7E-18) | 0.925 (8.5E-22) | 0.792 (7.3E-12) |
| v0.1 vs. SFR | 0.938 (8.9E-24) | 0.935 (2.7E-23) | 0.788 (1.1E-11) |
| v84.1 vs. SFR | 0.760 (1.5E-10) | 0.735 (1.2E-09) | 0.787 (1.3E-11) |
| v97.7 vs. SFR | 0.889 (6.5E-18) | 0.885 (1.6E-17) | 0.756 (2.3E-10) |
| v99.9 vs. SFR | 0.921 (2.5E-21) | 0.894 (2.2E-18) | 0.731 (1.7E-09) |
|
|
|||
| σ vs. M∗ | 0.810 (9.9E-13) | 0.752 (3.0E-10) | 0.810 (1.1E-12) |
| v15.9 vs. M∗ | 0.832 (7.0E-14) | 0.790 (9.4E-12) | 0.802 (2.7E-12) |
| v2.3 vs. M∗ | 0.808 (1.3E-12) | 0.730 (1.8E-09) | 0.808 (1.3E-12) |
| v0.1 vs. M∗ | 0.678 (6.2E-08) | 0.638 (6.3E-07) | 0.807 (1.4E-12) |
| v84.1 vs. M∗ | 0.886 (1.3E-17) | 0.820 (3.4E-13) | 0.792 (7.3E-12) |
| v97.7 vs. M∗ | 0.810 (1.1E-12) | 0.754 (2.5E-10) | 0.815 (6.2E-13) |
| v99.9 vs. M∗ | 0.566 (1.9E-05) | 0.657 (2.2E-07) | 0.811 (8.8E-13) |
|
|
|||
| σ vs. sSFR | 0.175 (0.22) | 0.246 (0.085) | 0.059 (0.69) |
| v15.9 vs. sSFR | 0.069 (0.64) | 0.142 (0.33) | 0.094 (0.52) |
| v2.3 vs. sSFR | 0.159 (0.27) | 0.268 (0.059) | 0.054 (0.71) |
| v0.1 vs. sSFR | 0.332 (0.019) | 0.371 (0.0081) | 0.051 (0.73) |
| v84.1 vs. sSFR | −0.044 (0.76) | −0.002 (0.99) | 0.070 (0.63) |
| v97.7 vs. sSFR | 0.160 (0.27) | 0.207 (0.15) | 0.019 (0.90) |
| v99.9 vs. sSFR | 0.435 (0.0016) | 0.314 (0.026) | −0.005 (0.97) |
Notes. This table lists the Spearman rank correlation coefficients (ρ ∈ (0.1)) and corresponding two-sided p-values calculated for the relationships between LoSVD parameters (velocity dispersion and percentile velocities) and galaxy properties (SFR, M∗, sSFR) that are shown in Figs. 14, 15 and Figs. A.1–A.5. A high value of ρ (e.g. ρ ≳ 0.5) combined with a low p-value (≤0.05) indicates the presence of a statistically significant correlation.
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