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Table 3.
Bayesian evidences from the GALPAK3D fits.
| ID | I(r) | v(r) | Prior | ln𝒵 | Δln𝒵 |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| 3 | Sérsic | DC14.MGE | 17 317 | 0 | |
| 3 | Sérsic | NFW.MGE | M⋆, SED | 17 312 | −5 |
| 15 | Sérsic | DC14.MGE | 8019 | 0 | |
| 15 | Sérsic | NFW.MGE | M⋆, SED | 8023 | +4 |
| 37 | Sérsic | DC14.MGE | 9514 | 0 | |
| 37 | Sérsic | NFW.MGE | M⋆, SED | 9651 | +137 |
| 912 | Sérsic | DC14.MGE | i⋆ | 8829 | 0 |
| 912 | Sérsic | NFW.MGE | i⋆, M⋆, SED | 8931 | +102 |
| 919 | Sérsic+B | DC14.Freeman | i⋆ | 27 552 | 0 |
| 919 | Sérsic+B | NFW.Freeman | i⋆, M⋆, SED | 27 915 | +363 |
| 937 | Sérsic | DC14.MGE | 8632 | 0 | |
| 937 | Sérsic | NFW.MGE | M⋆, SED | 8625 | −7 |
| 982 | Sérsic | DC14.MGE | 6736 | 0 | |
| 982 | Sérsic | NFW.MGE | M⋆, SED | 7040 | +304 |
| 943 | Sérsic | DC14.MGE | 15 374 | 0 | |
| 943 | Sérsic | NFW.MGE | M⋆, SED | 15 372 | −2 |
| 1002 | Sérsic | DC14.Freeman | 8151 | 0 | |
| 1002 | Sérsic | NFW.Freeman | M⋆, SED | 8155 | +4 |
Notes. (1) Galaxy ID; (2) Surface brightness profile; (3) Kinematic model (DM/Baryon); (4) External prior used; (5) Evidence lnZ on the deviance scale; (6) Bayesian factor between ‘NFW’ and the ‘DC14’ models (see Sect. 3.2).
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