Table A.1.
Properties of the discussed and depicted stellar objects identified at redshift z = 0 and shown in Fig. A.1.
| Galaxy (ID) | Host (ID) | Mstellar [M⊙] | Mgas [M⊙] | Mdm/Mbaryonic | κrot | shost [kpc] |  |
 |
|---|---|---|---|---|---|---|---|---|
| 878 | 138 | 6.7 × 107 | 1.4 × 109 | 0.0 | 0.47 | 94 | 9.7 | ( + 0.812, −0.0896, +0.576) |
| 1683 | 138 | 5.7 × 107 | 5.6 × 108 | 0.0 | 0.39 | 49 | 5.1 | ( + 0.936, −0.0479, +0.350) |
| 404872 | 404871 | 1.1 × 109 | 2.1 × 109 | 4.5 | 0.66 | 115 | 7.0 | (−0.712, +0.225, +0.665) |
| 404873 | 404871 | 8.0 × 106 | 1.8 × 109 | 0.020 | 0.39 | 157 | 9.5 | ( + 0.0415, −0.0105, −0.994) |
| 404879 | 404871 | 2.2 × 107 | 3.0 × 108 | 0.019 | 0.37 | 182 | 11 | ( + 0.0831, −0.0204, −0.996) |
| 404882 | 404871 | 1.7 × 107 | 2.5 × 108 | 0.0 | 0.41 | 193 | 12 | (−0.0283, −0.158, −0.987) |
Notes. Listed are the identification number of the stellar object, the identification number of its host galaxy, the stellar mass, Mstellar, gas mass, Mgas, the fraction of dark matter-to-baryonic matter, Mdm/(Mgas + Mstellar) = Mdm/Mbaryonic, the morphological parameter, κrot, the 3D separation between the stellar object and its host galaxy, shost, the fraction of this separation to the stellar half-mass radius of the host galaxy, 
, and the normalized specific orbital angular momentum, 
(Eq. (2)).
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