1 ID
2-3 RA, Dec
4-5 UDS K-band x,y (0.1342 arcsec pixels)
6-13 SExtractor output
14-85 Photometry in 12 bands (AB magnitudes, from 2-arcsec diameter apertures, corrected to total)
86 Mask flag (see main page for details)
87 Spectroscopic redshift, if available
88 Number of filters used to determine photo-z (minimum of 5 required)
89-104 EAZY photo-z output
105 EAZY prior used (K-band mag if available, otherwise R, otherwise None)
106 Saturated flag (Boolean); identifies objects saturated in Subaru imaging
107 Chi^2 of the best-fitting z=0 stellar template
108-111 Parameters associated with star/galaxy separation
112-123 Absolute magnitudes in all UDS filters based on redshift z_p
124-147 Lower and upper bounds on absolute magnituides
148 Redshift used for stellar masses (z_spec, otherwise z_p)
149-160 Stellar masses assuming a range of metallicities, as defined in BC03. Chi^2 fits for each metallicity are also provided.
161-172 Upper and lower bounds on the stellar masses for each metallicity
173 Stellar mass marginalised over all metallicities
174 Boolean column to identify candidate galactic stars
175 Boolean column to identify WFCAM cross-talk (or objects contaminated by cross-talk)
176 Boolean "good" flag, identifying objects in unmasked regions of optical/IR images with reliable 12-band photometry (see main page). Cross-talk are removed.
177 Boolean "best" flag, identifying objects in unmasked regions of optical/IR images with reliable 12-band photometry and deepest IRAC (see main page). Cross-talk are removed.
178 Boolean "good galaxies"; subset of "good" with candidate stars removed
179 Boolean "best galaxies"; subset of "best" with candidate stars removed