Table 1.
Modeling results with KINEMETRY.
| ——— Number of galaxies ——— | |||
|---|---|---|---|
| Kinematic | Parent | KINEMETRY | Asymmetric |
| map | sample | analyzed | (Iasym ≥ 0.05) |
| (1) | (2) | (3) | (4) |
| Stars | 8471 | 5245 | 1465 (27.9± 0.6%) |
| Gas (Hα) | 8471 | 4597 | 1322 (28.8 ± 0.7%) |
| Stars & Gas | 8471 | 3162 | 351 (11.1 ± 0.6%) |
| Stars only | 8471 | 2083 | 1079 (53.5 ± 1.1%) |
| Gas only | 8471 | 1435 | 867 (67.7 ± 1.2%) |
| Stellar kinematic map | |||
| Centrals | 5769 | 3633 | 1046 (28.8 ± 0.8%) |
| Satellites | 2579 | 1612 | 419 (26.0 ± 1.1%) |
| Gaseous kinematic map | |||
| Centrals | 5769 | 3431 | 908 (26.5 ± 0.8%) |
| Satellites | 2579 | 1166 | 414 (35.5 ± 1.4%) |
Notes. As the primary criterion, all galaxies considered in this work have environmental information available from Y07 or Argudo-Fernández et al. (2015). The percentages in Col. (4) represent the fraction of asymmetric galaxies relative to the valid sample (i.e., galaxies with > 90% of valid spaxels shown in Col. 3), along with the corresponding binomial errors. The final number of galaxies with more than 90% of valid spaxels (S/Nspx > 5) within 1 Reff is 6680, of which 4681 are centrals and 1999 are satellites.
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