Open Access
Table E.1.
Description of the columns included in the catalogue associated with this paper.
| Column | Label | Description |
|---|---|---|
| 1 | CLUSTER | Name of the lensing cluster |
| 2 | ID_R21 | Source ID from the MUSE Atlas of Lensing Clusters R21 |
| 3 | ID_HFFDS | Source ID from the HFF-DeepSpace catalogue (Shipley et al. 2018) |
| 4 | RA | Right ascension (J2000) of the morphological centre in decimal degrees |
| 5 | DEC | Declination (J2000) of the morphological centre in decimal degrees |
| 6 | Z_R21 | Systemic redshift from R21 |
| 7 | MU_R21 | Lensing magnification from R21 |
| 8 | S/N_MAX | S/N of the brightest [O II] spaxel |
| 9 | R_PSF | MUSE PSF radius in arcseconds |
| 10 | EFF_RADIUS | Effective radius from a single-Sérsic fit to the F160W flux in arcseconds |
| 11 | INCLINATION | Inclination from a single-Sérsic fit to the F160W flux in degrees |
| 12 | B/T_FLUX | Bulge-to-total flux ratio in the F160W band |
| 13 | LOG_MSTAR_16 | 16th percentile of the log(M★/M⊙) posterior |
| 14 | LOG_MSTAR_MED | Median of the log(M★/M⊙) posterior |
| 15 | LOG_MSTAR_84 | 84th percentile of the log(M★/M⊙) posterior |
| 16 | LOG_SFR_16 | 16th percentile of the log(SFR/[M⊙/yr]) posterior |
| 17 | LOG_SFR_MED | Median of the log(SFR/[M⊙/yr]) posterior |
| 18 | LOG_SFR_84 | 84th percentile of the log(SFR/[M⊙/yr]) posterior |
| 19 | LOG_MHI | Logarithm of the atomic gas mass (in M⊙, including Helium) inferred from scaling relations |
| 20 | LOG_MMOL | Logarithm of the molecular gas mass (in M⊙) inferred from scaling relations |
| 21 | LOG_MBAR | Logarithm of the total baryonic mass (in M⊙) |
| 22 | LOG_V1.8_MED | Median of the log(v1.8 [km s−1]) posterior |
| 23 | LOG_V1.8_STD | Standard deviation of the log(v1.8 [km s−1]) posterior |
| 24 | LOG_V2.0_MED | Median of the log(v2.0/[km s−1]) posterior |
| 25 | LOG_V2.0_STD | Standard deviation of the log(v2.0 [km s−1]) posterior |
| 26 | SIG0_MED | Median of the σ0 posterior in km s−1 |
| 27 | SIG0_STD | Standard deviation of the σ0 posterior in km s−1 |
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