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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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