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Table A.2.

Description of the columns of the MAGIC galaxy catalog.

Col. name Description
ID MAGIC object ID, of the form X_CGrY, where X is the identifier within the fields corresponding to COSMOS group CGrY
C2015_ID Object ID in the COSMOS2015 catalog (Laigle et al. 2016)
FIELD Name of the MAGIC field, see Table 1
RA Right ascension (J2000, degrees), see Sect. 2.3, adjusted with the morphology analysis (Mercier et al. 2023), when available
DEC Declination in (J2000, degrees), see Sect. 2.3, adjusted with the morphology analysis (Mercier et al. 2023), when available
Z Systemic redshift of the source, adjusted with the kinematics analysis (Mercier et al. 2023), when available, see Sect. 3.1

CONFID Redshift confidence level from 1 (low) to 3 (high), see Sect. 3.1
LMS Logarithm of stellar mass M (in M) within 3″ diameter apertures estimated from SED fitting with CIGALE, see Sect. 2.4
DLMS Uncertainty on the logarithm of stellar mass (in M) within 3″ diameter apertures
LSFR Logarithm of SFR (in M yr−1) within 3″ diameter apertures estimated from SED fitting with CIGALE, see Sect. 2.4
DLSFR Uncertainty on the logarithm of SFR (in M yr−1) within 3″ diameter apertures
E(B-V) Color excess estimated from SED fitting with CIGALE, see Sect. 2.4
NUV-RP NUV − r+ rest-frame color estimated from SED fitting with CIGALE, see Sect. 2.4
RP-J r+ − J rest-frame color estimated from SED fitting with CIGALE, see Sect. 2.4

MGR_ID MAGIC group ID to which the galaxy belongs, as defined in the group catalog, see Table A.1
VMC_D Galaxy density Σ in log (Mpc−2) at the location of the galaxy inferred from the VMC method, see Sect. 4.3
VMC_OD Galaxy over-density (1 + δ) in log at the location of the galaxy inferred from the VMC method, see Sect. 4.3
VOR_D Galaxy density in log (Mpc−2) at the location of the galaxy inferred from Voronoi tessellations, see Sect. 4.4
DR Distance to group center Δr (kpc), see Sect. 4.5
DV Velocity Δv (km s−1) in the frame of the group with respect to the group redshift, see Sect. 4.5
ETA Phase space parameter η, see Sect. 4.5

Notes. Stars are included in the catalog, but their physical and environment properties are not computed. Such properties are not provided either for the 788 galaxies without MUSE redshift determination.

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