Table 2.
Median and 68% confidence level (CL) of the posterior distributions of the parameters ma, Mc, c, Mh, and M⋆, and the reduced chi-square of the maximum posterior fit to the LTs catalog, including some of the rogues.
| Galaxy | M⋆ | ma | Mc | Mh | c |  |
rc | rt | 103 × ρc |
|---|---|---|---|---|---|---|---|---|---|
| [107 M⊙] | [10−23 eV] | [108 M⊙] | [1010 M⊙] | kpc | kpc | M⊙/pc3 | |||
| NGC 2366 |
 |
 |
 |
 |
 |
1.29 |
 |
 |
 |
| DDO 168 |
 |
 |
 |
 |
 |
0.56 |
 |
4.69† |
 |
| DDO 52 |
 |
 |
 |
 |
 |
0.13 |
 |
 |
 |
| DDO 87 |
 |
 |
 |
 |
 |
0.27 |
 |
 |
 |
| DDO 126 |
 |
 |
 |
 |
 |
0.49 |
 |
3.3† |
 |
| WLM |
 |
 |
 |
 |
 |
0.68 |
 |
 |
 |
| DDO 154 |
 |
 |
 |
 |
 |
0.94 |
 |
 |
 |
| UGC 8508 |
 |
 |
 |
 |
 |
0.083 |
 |
1.39† |
 |
| CvnIdwA |
 |
 |
 |
 |
 |
0.43 |
 |
1.57† |
 |
| DDO 210 |
 |
 |
 |
 |
 |
0.71 |
 |
0.44† |
 |
| – rogues – | |||||||||
| DDO 50 |
 |
 |
 |
 |
 |
0.53 |
 |
 |
 |
| DDO 133 |
 |
 |
 |
 |
 |
0.33 |
 |
 |
 |
| NGC 6822* |
 |
 |
 |
 |
 |
1.84 |
 |
 |
 |
Notes. We also include the derived core radius, transition radius and central density of the distribution. We flag the galaxy NGC 6822 with * because it was not initially selected as a rogue galaxy (see text for details). The transition radii with an upper uncertainty equal to 0 indicates that less than 84% of the posterior distribution lies below the maximum observable radius rmax, while for those not showing an uncertainty band and marked by †, at least 84% of the posterior distribution lies above rmax.
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