Table 4
Kinematics and close environment classification of MASSIV “first epoch” sample galaxies.
| VVDS ID | S/N |
|
ΔPA [°] |
|
Vmax/σ | Shear | Rotator | Isolated | Isolation flag |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
|||||||||
| 020106882 | 7.6 | 1.2 | 23 ± 4 | 0.07 | 3.2 | High | Yes | Yes | B |
| 020116027 | 8.2 | 1.3 | 23 ± 6 | 0.27 | 0.6 | Low | No | No | A |
| 020126402 | < 3 | − | − | − | − | − | − | − | − |
| 020147106 | 12.2 | 1.4 | 7 ± 3 | 0.18 | 0.3 | Low | Yes | Yes | B |
| 020149061 | 6.2 | 0.7 | 34 ± 90 | 0.17 | 1.5 | Low | Yes | Yes | B |
| 020164388 | 11.0 | 1.2 | 65 ± 5 | 0.11 | 1.5 | Low | No | Yes | B |
| 020167131 | 3.7 | 0.3 | 87 ± 11 | 0.22 | 5.0 | Low | No | No | A |
| 020182331 | 6.1 | 0.9 | 34 ± 6 | 0.09 | 2.0 | High | No | Yes | B |
| 020193070 | 4.9 | 0.8 | 31 ± 3 | 0.10 | 3.6 | High | No | Yes | B |
| 020208482 | 4.1 | 0.3 | 20 ± 12 | 0.18 | 22.9 | Low | Yes | Yes | B |
| 020214655 | 7.5 | 0.8 | 51 ± 5 | 0.17 | 0.8 | Low | No | Yes | B |
| 020217890 | <3 | − | − | − | − | − | − | − | − |
| 020239133 | 5.3 | 0.8 | 14 ± 6 | 0.11 | 2.0 | High | Yes | Yes | B |
| 020240675 | 5.5 | 0.5 | 7 ± 18 | 0.40 | 1.5 | Low | No | Yes | B |
| 020255799 | 4.5 | 0.6 | 75 ± 77 | 1.04 | 0.2 | Low | No | Yes | B |
| 020261328 | 7.8 | 1.0 | 8 ± 8 | 0.07 | 2.4 | High | Yes | Yes | B |
| 020278667 | 4.1 | 0.2 | 35 ± 14 | 0.34 | 1.5 | Low | No | Yes | C |
| 020283083 | 7.0 | 0.9 | 58 ± 5 | 0.18 | 1.5 | Low | No | No | B |
| 020283830 | 4.8 | 1.2 | 14 ± 2 | 0.08 | 11.3 | High | Yes | No | B |
| 0202940451 | 7.0 | 1.2 | 2 ± 4 | 0.12 | 3.9 | Low | No | No | B |
| 020306817 | <3 | − | − | − | − | − | − | − | − |
| 020363717 | 11.4 | 1.1 | 49 ± 8 | 0.19 | 0.5 | Low | No | Yes | B |
| 020370467 | 5.5 | 0.9 | 31 ± 27 | 0.45 | 0.6 | Low | No | Yes | B |
| 020386743 | 8.8 | 0.9 | 67 ± 8 | 0.26 | 0.8 | Low | No | No | A |
| 020461235 | 5.8 | 1.1 | 19 ± 4 | 0.10 | 3.5 | High | Yes | No | B |
| 020461893 | 7.0 | 1.3 | 4 ± 5 | 0.10 | 0.9 | Low | Yes | Yes | B |
| 020465775 | 6.8 | 0.7 | 31 ± 5 | 0.24 | 0.8 | Low | No | No | B |
| 140083410 | 6.0 | 1.0 | 88 ± 12 | 0.35 | 0.4 | Low | No | Yes | A |
| 140096645 | 10.3 | 1.0 | 20 ± 90 | 0.07 | 3.9 | High | Yes | No | B |
| 140123568 | 3.5 | 0.1 | 43 ± 90 | 0.44 | 0.7 | Low | No | Yes | B |
| 140137235 | 3.2 | 0.1 | 8 ± 29 | 0.11 | 3.5 | Low | Yes | Yes | B |
| 140217425 | 6.8 | 1.9 | 2 ± 1 | 0.04 | 7.1 | High | Yes | Yes | B |
| 140258511 | 8.1 | 1.3 | 52 ± 42 | 0.12 | 5.1 | High | Yes | Yes | A |
| 140262766 | 6.5 | 1.0 | 32 ± 28 | 0.07 | 3.1 | High | Yes | Yes | B |
| 140545062 | 8.5 | 1.3 | 14 ± 41 | 0.06 | 3.1 | High | Yes | Yes | B |
| 220014252 | 11.0 | 1.7 | 5 ± 2 | 0.08 | 1.4 | High | Yes | Yes | B |
| 220015726 | 10.4 | 1.0 | 8 ± 12 | 0.04 | 3.7 | High | Yes | Yes | B |
| 220071601 | <3 | − | − | − | − | − | − | − | − |
| 220148046 | 4.0 | 0.4 | 25 ± 18 | 0.39 | 0.9 | Low | No | Yes | C |
| 220376206 | 12.6 | 2.4 | 10 ± 1 | 0.05 | 2.8 | High | Yes | No | B |
| 220386469 | 4.5 | 1.1 | 17 ± 12 | 0.42 | 0.9 | Low | No | Yes | B |
| 220397579 | 15.7 | 2.0 | 31 ± 10 | 0.68 | 0.2 | Low | No | No | A |
| 220397579s | 5.4 | 1.2 | 11 ± 3 | 0.06 | 8.3 | High | Yes | No | A |
| 220544103 | 10.4 | 1.2 | 11 ± 55 | 0.07 | 1.9 | High | Yes | No | B |
| 220544394 | 10.5 | 1.1 | 54 ± 7 | 0.08 | 1.1 | Low | No | No | A |
| 220576226 | 11.6 | 1.3 | 45 ± 15 | 0.15 | 0.6 | Low | No | Yes | B |
| 220578040 | 5.9 | 1.4 | 10 ± 14 | 0.08 | 4.9 | High | Yes | Yes | C |
| 220584167 | 13.8 | 2.1 | 15 ± 2 | 0.04 | 4.8 | High | Yes | Yes | B |
| 220596913 | 5.7 | 6.2 | 8 ± 1 | 0.09 | 3.7 | High | Yes | Yes | B |
| 910193711 | 6.0 | 1.8 | 30 ± 4 | 0.22 | 0.8 | Low | No | Yes | C |
| 910279515 | 3.5 | 1.5 | 23 ± 8 | 0.11 | 3.9 | High | Yes | Yes | C |
Notes. Column (2) gives the average S/N of the S/N map. The size of the galaxy with respect to the seeing is given in Col. (3). The criteria used to determine if galaxies are in rotation or not (8) are the mismatch between morphological and kinematic position angles (4) and the residuals normalized by the velocity shear (5). The ratio of the rotation velocity over the local velocity dispersion is given in Col. (6). Galaxies are classified according the observed velocity shear in Col. (7): galaxies with Vshear < 100 km s-1 or Vshear > 100 km s-1 are respectively classified as low and high shear. The close environment classification and its associated quality flag are given in (9) and (10). The suffix “s” refers to secondary objects which have been detected both in Hα and in the I-band image.
This galaxy is classified as non-rotating even if it fulfils the criteria because the kinematics seem to indicate that this system is composed of two close companions (cf. Appendix A).
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