Table 4.
Best-fit kinematic parameters for the galaxies in our sample.
| HATLAS090750 | HATLAS114625 | HATLAS121446 | |
|---|---|---|---|
| iCO (deg) | 65 | 70 | 80 |
| PACO (deg) | −132 ± 1 | −76 ± 1 | −10 ± 1 |
| R1/2, CO (kpc) | 1.44 ± 0.01 | 2.09 ± 0.01 | 2.74 ± 0.01 |
| Vrot, CO (km s−1) | 67 ± 2 | 198 ± 22 | 245 ± 5 |
| σv, CO (km s−1) | 35 ± 12 | 26 ± 10 | 34 ± 11 |
 |
11.2 | 10.4 | 7.0 |
| iPaα (deg) | 65 | 70 | 80 |
| PAPaα (deg) | −123 ± 1 | −81 ± 1 | −9 ± 1 |
| R1/2, Paα (kpc) | 2.10 ± 0.05 | 1.72 ± 0.01 | 2.52 ± 0.03 |
| Vrot, Paα (km s−1) | 68 ± 4 | 190 ± 7 | 246 ± 9 |
| σv, Paα (km s−1) | 66 ± 18 | 51 ± 30 | 51 ± 31 |
 |
7.1 | 5.0 | 7.8 |
Notes. PA is the kinematic major-axis position angle. R1/2 is the half-light radius corrected by beam-smearing effects. σv is the global velocity dispersion value (see Sect. 3.2.2). Vrot is the rotational velocity measured across the major kinematic axis. i is the inclination angle (for a face-on galaxy, i = 0 deg). We do not give uncertainty estimates for i as it is constrained by the K-band image model. The “CO” and “Paα” sub-indices indicate the emission line from which the kinematic parameters were estimated.
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