Table 2.
Kinematics results from the GALPAK3D fits with our disk-halo decomposition.
| ID | nO2 | iO2 | ReO2 | Model | σ0 | Vvir | cvir, −2 | log M⋆/M⊙ | log Mvir/M⊙ | ln𝒵 | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (kpc) | (km s−1) | (km s−1) | ||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | |
| 3 (a) | 0.75 ± 0.05 | 65 ± 1 | 6.4 ± 0.1 | DC14.MGE | 27 ± 3 | 122 ± 12 | 12 ± 2 | 10.02 ± 0.23 | 11.71 ± 0.12 | 17 317 (d) | |
| 15 | 0.6 ± 0.1 | 63 ± 1 | 6.0 ± 0.2 | DC14.MGE | 35 ± 2 | 115 ± 15 | 15 ± 2 | 10.19 ± 0.27 | 11.61 ± 0.16 | 8019 | |
| 37 | 0.9 ± 0.1 | 55 ± 1 | 3.7 ± 0.1 | DC14.MGE | 25 ± 3 | 143 ± 35 | 6.6 ± 1 | 8.89 ± 0.30 | 11.80 ± 0.32 | 9514 | |
| 912 (b) | 0.5 ± 0.1 | 35 | 2.4 ± 0.1 | DC14.MGE | 27 ± 3 | 154 |
17 ± 2 | 9.34 ± 0.21 | 12.01 ± 0.25 | 8829 | |
| 919 (b) | 0.6 ± 0.1 | 35 | 3.6 ± 0.1 | DC14.Freeman | 39 ± 2 | 122 ± 15 | 16 ± 1 | 9.53 |
11.54 ± 0.16 | 27 552 (d) | |
| 937 (c) | 0.5 ± 0.1 | 84 ± 1 | 7.1 ± 0.1 | NFW.MGE | 18 ± 5 | 112 ± 13 | 9 ± 1 | 9.29 |
11.56 ± 0.16 | 8632 | |
| 943 | 1.0 ± 0.1 | 72 ± 1 | 4.8 ± 0.1 | DC14.MGE | 48 ± 2 | 89 ± 6 | 15 ± 4 | 9.97 |
11.27 ± 0.09 | 15 374 (d) | |
| 982 | 1.2 ± 0.1 | 63 ± 1 | 5.4 ± 0.3 | DC14.MGE | 35 ± 3 | 203 |
7 ± 1 | 9.57 ± 0.25 | 12.22 |
6736 | |
| 1002 | 0.95 ± 0.5 | 70 ± 1 | 3.9 ± 0.1 | DC14.Freeman | 36 ± 2 | 122 |
7 ± 1 | 9.67 |
11.60 |
8151 |
Notes. (1) Galaxy ID; (2) Sérsic index from MUSE data ([O II]); (3) Inclination from [O II]; (4) Half-light radius from [O II]; (5) Model used for the disk-halo decomposition; (6) Velocity dispersion σ0 (see text); (7) Virial velocity Vvir for the DM halo component; (8) Halo concentration parameter cvir; (9) Stellar mass M⋆ from GALPAK3D; (10) Halo mass Mvir; (11) Logarithm of the evidence 𝒵. The quoted errors are 2σ (95%).
This galaxy is located on the edge of the MXDF deep footprint, and we use the deeper data in the UDF10 pointing from Bacon et al. (2017).
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