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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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