Open Access
Table E.1
Column description of the REGALADE catalog.
| Column | Unit | Description |
|---|---|---|
| name | Identifier from the best distance catalog (ref_D_in) | |
| ra | deg | Right Ascension |
| dec | deg | Declination |
| id_cat | Bitwise flag identifying matched catalogs | |
| R1 | arcsec | Semimajor axis of ellipse |
| R2 | arcsec | Semiminor axis of ellipse |
| PA | deg | Position angle of ellipse |
| ref_ell | Index of the catalog used for R1, R2, PA(1) | |
| n_dist | Number of distance estimates | |
| D | Mpc | Final recommended distance |
| z | Final recommended redshift | |
| D_input | Mpc | Best available distance |
| D_err | Mpc | Error on the best available distance |
| ref_D_in | Index of the catalog used for D_input(1) | |
| D_min | Mpc | Minimum of available distances |
| D_max | Mpc | Maximum of available distances |
| D_std | Mpc | Standard deviation of available distances |
| D_tmean | Mpc | Trimmed mean of available distances |
| G | mag | Gaia G magnitude |
| BP | mag | Gaia BP magnitude |
| PM | mas/yr | Gaia proper motion |
| angDist | arcsec | Separation to Gaia match |
| rpsf | mag | r-band PSF magnitude |
| gmag | mag | g-band Kron magnitude |
| rmag | mag | r-band Kron magnitude |
| imag | mag | i-band Kron magnitude |
| zmag | mag | z-band Kron magnitude |
| W1mag | mag | WISE W1 magnitude |
| W2mag | mag | WISE W2 magnitude |
| griz_ref | Catalog used for optical photometry(2) | |
| W_ref | Catalog used for infrared photometry(3) | |
| dK | mag | 2MASS extended source K magnitude correction |
| EBV | mag | Color excess interpolated from Schlegel et al. (1998) |
| logM | M⊙ | log of the stellar mass |
| f_reliability | Flag galaxies exclusively in lower reliability catalogs | |
| frac_nearby | Fraction of annotators that voted "nearby galaxy" |
Notes.(1) Index as reported in Table 1. (2)The griz_ref column takes values as follows; 0: none, 1: Pan-STARRS, 2: DELVE, 3: LS DR9, 4: LS DR10. (3)The W_ref column takes values as follows; 0: none, 1: AllWISE, 3: LS DR9, 4: LS DR10.
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