Table C.1.
Parameters estimated from a 2D Gaussian fit of the flux maps, virial mass estimates, and the results of the spectroastrometry method.
| No. (a) | Object ID | FWHMmaj(b) | FWHMmin(c) | Rem | Mvir | rspec | μspec |
|---|---|---|---|---|---|---|---|
| (mas) | (mas) | (kpc) | (1010 M⊙) | (kpc) | (1010 M⊙) | ||
| 2 | VHS J2101−5943 | POINT-LIKE SOURCE | <8.34 | <8.0 | <2.3 | <2.6 | |
| 6 | SDSS J1328−0224 | 339 ± 50 | 189 ± 35 |
 |
 |
0.3 ± 0.2 | 0.5 ± 0.3 |
| 7 | SDSS J0923+0247 | 385 ± 50 | 340 ± 58 |
 |
 |
0.7 ± 0.1 | 1.8 ± 0.4 |
| 9 | SDSS J0129−0035 | 303 ± 51 | 271 ± 59 |
 |
 |
0.37 ± 0.06 | 0.30 ± 0.06 |
| 10 | SDSS J1044−0125 | POINT-LIKE SOURCE | <1.38 | <4.8 | 0.4 ± 0.3 | 1.8 ± 1.5 | |
| 11 | SDSS J1306+0356 | 1290 ± 430 | 410 ± 240 |
 |
 |
1.1 ± 0.7 | 1.4 ± 0.9 |
| 12 | SDSS J2310+1855 | 512 ± 61 | 287 ± 135 |
 |
 |
0.41 ± 0.07 | 1.4 ± 0.3 |
| 14 | SDSS J2054−0005 | 352 ± 72 | 293 ± 97 |
 |
 |
0.33 ± 0.08 | 0.45 ± 0.12 |
| 19 | ULAS J1319+0950 | 536 ± 95 | 328 ± 78 |
 |
 |
0.64 ± 0.12 | 3.5 ± 1.0 |
| 25 | PSO J183+05 | 604 ± 63 | 477 ± 52 |
 |
 |
0.44 ± 0.12 | 1.5 ± 0.5 |
| 26 | PSO J167−13 | 1068 ± 74 | 467 ± 53 |
 |
 |
1.16 ± 0.12 | 6.7 ± 1.0 |
Notes.
Source identification numbers in agreement with those listed in the first column of Table 1.
,Major and minor FWHM of the 2D best-fit Gaussian of the flux maps deconvolved from the beam. Point-like sources are explicitly indicated. In these cases, minor FWHM of the synthesised beam is taken as upper limit on the angular dimension of the emitting region. Uncertainties on quantities are statistical errors ignoring any possible systematic biases.
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