Table 3
Kinematic properties.
| Objects |  |
 |
 |
υobs,lim∕σint | υobs,lim∕σ0,lim | |
|---|---|---|---|---|---|---|
| [km s−1] | [km s−1] | [km s−1] | ||||
| AS1063-1816 | 44 ± 3 | – | – | – | – | |
| AS1063-658 | 62 ± 4 | 32 ± 9 | 63 ± 10 | 1.01 | 1.97 | |
| AS1063-1611 | 48 ± 2 | – | – | – | – | |
| AS1063-1670 | 119 ± 27 | 32 ± 12 | 80 ± 10 | 0.67 | 2.5 | |
| AS1063-1152 | 53 ± 4 | 40 ± 8 | 80 ± 11 | 1.51 | 2.0 | |
| AS1063-1321 | 52 ± 5 | 35 ± 7 | 65 ± 8 | 1.25 | 1.86 | |
| AS1063-1331 | 60 ± 5 | – | – | – | – | |
| AS1063-732 | 79 ± 6 | 50 ± 10 | 81 ± 15 | 1.03 | 1.62 | |
| AS1063-1904 | 55 ± 4 | 66 ± 9 | 22 ± 5 | 0.39 | 0.33 | |
| AS1063-606_1 | 40 ± 5 | 31 ± 6 | 12 ± 5 | 0.3 | 0.39 | |
| AS1063-942 | 40 ± 4 | 32 ± 6 | 31 ± 8 | 0.78 | 0.97 | |
| AS1063-885d | 31 ± 11 | – | – | – | – | |
| AS1063-1720 | 105 ± 54 | 52 ± 25 | 37 ± 10 | 0.35 | 0.71 | |
| MACS1206-2005 | 104 ± 8 | 82 ± 15 | 90 ± 7 | 0.86 | 1.1 | |
| MACS1206-1123 | 35 ± 4 | – | – | – | – | |
| MACS1206-1409d | 40 ± 22 | – | – | – | – | |
| MACS1206-1235 | 59 ± 29 | – | – | – | – | |
| MACS1206-445d | 71 ± 15 | – | – | – | – | |
| MACS1206-415 | 78 ± 20 | – | – | – | – | |
| MACS1206-1622 | 48 ± 5 | – | – | – | – | |
| MACS1206-2372 | 58 ± 29 | – | – | – | – | |
| MACS1206-1616_1 | 77 ± 20 | 79 ± 24 | 81 ± 7 | 1.05 | 1.02 | |
| MACS1206-1472 | 82 ± 7 | 62 ± 13 | 63 ± 6 | 0.77 | 1.02 | |
| MACS1206-820 | 96 ± 23 | – | – | – | – |
Notes. (a) The integrated dispersion σint is the dispersion measured from the integrated spectrum corrected for instrumental broadening (see Eq. (2)). (b) The upper limit dispersion σ0,lim is the dispersion measured in the outer region on the major axis to avoid beam smearing effects and corrected for instrumental broadening. (c) The lower limit velocity υobs,lim is defined as the difference between the maximum and minimum velocity on the major axis divided by two, not corrected for inclination. When both Hα and [OIII] emission lines are detected for the same galaxy, we use Hα only to determine υobs,lim. (d) These three galaxies are unresolved.
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