Table E.1.
Column description of the catalogue used in this analysis.
| No. | Title | Description |
|---|---|---|
| 1 | ID | MUSE galaxy ID in the form X-CGrY, where X refers to the galaxy identification |
| number within the field targeting COSMOS group CGrY | ||
| 2 | z | Spectroscopic systemic redshift derived from the kinematics modelling |
| 3 | RA | J2000 Right Ascension of morphological centre in decimal degrees |
| 4 | Dec | J2000 Declination of morphological centre in decimal degrees |
| 5 | N | Number of galaxies in the host structure. Field galaxies have a value of -99. |
| 6 | R/R200 | Ratio of the projected distance of a galaxy to its host group’s centre with the radius of the |
| group R200 (see Sect. 2.3). Field galaxies have a value of -99. | ||
| 7 | dV/sigma | Ratio of the systemic velocity of a galaxy along the line-of-sight with its host group’s |
| velocity dispersion (see Sect. 2.3). Field galaxies have a value of -99. | ||
| 8 | Eta | Environmental tracer defined in Sect. 2.3, combining parameters 6 and 7. Field galaxies have |
| a value of -99. | ||
| 9 | log over-density | Logarithm of the over-density around the galaxies as measured by the VMC technique |
| (see the end of Sect. 2.3) | ||
| 10 | log j_HST_MM | Logarithm of the specific stellar angular momentum (kpc km s−1) derived from HST images |
| using the mass model rotation curve | ||
| 11 | log j_HST_flat | Logarithm of the specific stellar angular momentum (kpc km s−1) derived from HST images |
| using the flat model rotation curve | ||
| 12 | log j_exp_MM | Logarithm of the specific stellar angular momentum (kpc km s−1) derived by numerically |
| integrating Eq. 6 assuming an exponential disk mass distribution and a mass | ||
| model rotation curve | ||
| 13 | log j_exp_flat | Logarithm of the specific stellar angular momentum (kpc km s−1) analytically derived |
| assuming an exponential disk mass distribution and a flat model rotation curve (see | ||
| Appendix D) | ||
| 14 | Gas dispersion | Average velocity dispersion of the ionised gas (kpc km s−1) measured in the velocity dispersion map |
| of the [O II] doublet after correcting for the LSF and beam-smearing | ||
| 15 | log M* | Logarithm of the stellar mass (M⊙) |
Notes: The sample used in this catalogue corresponds to the 182 galaxies selected in terms of their surface, S/N, and stellar disk inclination (see Sect. 2.4). Complementary physical, morphological, and dynamical information can be found in the morpho-kinematics catalogue published in Mercier et al. (2022, catalogues can be cross-matched using the ID field). All logarithmic values are given as decimal logarithms.
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