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(The bold columns are indexed columns)
Column NameDescriptionDatatype
aProfile RMS along major axis (pixels)DOUBLE
apertureTotal-restricted Photometric Aperture (pixels)BIGINT
bProfile RMS along minor axis (pixels)DOUBLE
chi2Poorness of BPZ fit: observed vs. model fluxesDOUBLE
classMost probable classification: (3/6 = galaxy/star)BIGINT
decDeclination in decimal degreesDOUBLE
ef378_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef378_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef378_petroTotal magnitude uncertainty [AB]DOUBLE
ef395_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef395_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef395_petroTotal magnitude uncertainty [AB]DOUBLE
ef410_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef410_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef410_petroTotal magnitude uncertainty [AB]DOUBLE
ef430_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef430_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef430_petroTotal magnitude uncertainty [AB]DOUBLE
ef515_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef515_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef515_petroTotal magnitude uncertainty [AB]DOUBLE
ef660_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef660_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef660_petroTotal magnitude uncertainty [AB]DOUBLE
ef861_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ef861_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ef861_petroTotal magnitude uncertainty [AB]DOUBLE
eg_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
eg_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
eg_petroTotal magnitude uncertainty [AB]DOUBLE
ei_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ei_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ei_petroTotal magnitude uncertainty [AB]DOUBLE
elatEcliptic LatitudeDOUBLE
elonEcliptic LongitudeDOUBLE
er_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
er_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
er_petroTotal magnitude uncertainty [AB]DOUBLE
eujava_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
eujava_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
eujava_petroTotal magnitude uncertainty [AB]DOUBLE
ez_aperCircular-3arcsec-Diameter-Aperture magnitude uncertainty [AB]DOUBLE
ez_autoTotal-restricted magnitude uncertainty [AB]DOUBLE
ez_petroTotal magnitude uncertainty [AB]DOUBLE
f378_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f378_autoTotal-restricted magnitude [AB]DOUBLE
f378_petroTotal magnitude [AB]DOUBLE
f395_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f395_autoTotal-restricted magnitude [AB]DOUBLE
f395_petroTotal magnitude [AB]DOUBLE
f410_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f410_autoTotal-restricted magnitude [AB]DOUBLE
f410_petroTotal magnitude [AB]DOUBLE
f430_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f430_autoTotal-restricted magnitude [AB]DOUBLE
f430_petroTotal magnitude [AB]DOUBLE
f515_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f515_autoTotal-restricted magnitude [AB]DOUBLE
f515_petroTotal magnitude [AB]DOUBLE
f660_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f660_autoTotal-restricted magnitude [AB]DOUBLE
f660_petroTotal magnitude [AB]DOUBLE
f861_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
f861_autoTotal-restricted magnitude [AB]DOUBLE
f861_petroTotal magnitude [AB]DOUBLE
flraddetFraction-of-light radii (pixels)DOUBLE
fwhmFull width at half maximum for detection image (pixels)DOUBLE
g_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
g_autoTotal-restricted magnitude [AB]DOUBLE
g_petroTotal magnitude [AB]DOUBLE
glatGalactic LatitudeDOUBLE
glonGalactic LongitudeDOUBLE
htm9HTM index (order 9 => ~10 arcmin size)INTEGER
i_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
i_autoTotal-restricted magnitude [AB]DOUBLE
i_petroTotal magnitude [AB]DOUBLE
idObject ID NumberCHAR
isoareaIsophotal area above Analysis thresholdBIGINT
krraddetKron apertures in units of A or B (pixels)DOUBLE
m_bAbsolute Magnitude [AB] (B_JOHNSON) for the First PeakDOUBLE
mumaxPeak Surface Brightness above background [mag x arcsec^{-2}]DOUBLE
nest4096HEALPIX index (Nside 4096, Ring scheme => ~52 arcsec size)INTEGER
oddsP(z) contained within zb +/- 2*0.015*(1+z) for the First PeakDOUBLE
photoflagSExtractor Photometric FlagBIGINT
prob_galProbability of being a galaxyDOUBLE
prob_starProbability of being a starDOUBLE
r_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
r_autoTotal-restricted magnitude [AB]DOUBLE
r_petroTotal magnitude [AB]DOUBLE
raRight Ascension in decimal degreesDOUBLE
random_idRandom ID in the range 0.0 => 100.0REAL
ring256HEALPIX index (Nside 256, Ring scheme => ~14 arcmin size)INTEGER
s2n_f378_aperSignal-to-noise of the detection within F378_aperDOUBLE
s2n_f378_autoSignal-to-noise of the detection within F378_autoDOUBLE
s2n_f378_petroSignal-to-noise of the detection within F378_petroDOUBLE
s2n_f395_aperSignal-to-noise of the detection within F395_aperDOUBLE
s2n_f395_autoSignal-to-noise of the detection within F395_autoDOUBLE
s2n_f395_petroSignal-to-noise of the detection within F395_petroDOUBLE
s2n_f410_aperSignal-to-noise of the detection within F410_aperDOUBLE
s2n_f410_autoSignal-to-noise of the detection within F410_autoDOUBLE
s2n_f410_petroSignal-to-noise of the detection within F410_petroDOUBLE
s2n_f430_aperSignal-to-noise of the detection within F430_aperDOUBLE
s2n_f430_autoSignal-to-noise of the detection within F430_autoDOUBLE
s2n_f430_petroSignal-to-noise of the detection within F430_petroDOUBLE
s2n_f515_aperSignal-to-noise of the detection within F515_aperDOUBLE
s2n_f515_autoSignal-to-noise of the detection within F515_autoDOUBLE
s2n_f515_petroSignal-to-noise of the detection within F515_petroDOUBLE
s2n_f660_aperSignal-to-noise of the detection within F660_aperDOUBLE
s2n_f660_autoSignal-to-noise of the detection within F660_autoDOUBLE
s2n_f660_petroSignal-to-noise of the detection within F660_petroDOUBLE
s2n_f861_aperSignal-to-noise of the detection within F861_aperDOUBLE
s2n_f861_autoSignal-to-noise of the detection within F861_autoDOUBLE
s2n_f861_petroSignal-to-noise of the detection within F861_petroDOUBLE
s2n_g_aperSignal-to-noise of the detection within g_aperDOUBLE
s2n_g_autoSignal-to-noise of the detection within g_autoDOUBLE
s2n_g_petroSignal-to-noise of the detection within g_petroDOUBLE
s2n_i_aperSignal-to-noise of the detection within i_aperDOUBLE
s2n_i_autoSignal-to-noise of the detection within i_autoDOUBLE
s2n_i_petroSignal-to-noise of the detection within i_petroDOUBLE
s2n_r_aperSignal-to-noise of the detection within r_aperDOUBLE
s2n_r_autoSignal-to-noise of the detection within r_autoDOUBLE
s2n_r_petroSignal-to-noise of the detection within r_petroDOUBLE
s2n_ujava_aperSignal-to-noise of the detection within uJAVA_aperDOUBLE
s2n_ujava_autoSignal-to-noise of the detection within uJAVA_autoDOUBLE
s2n_ujava_petroSignal-to-noise of the detection within uJAVA_petroDOUBLE
s2n_z_aperSignal-to-noise of the detection within z_aperDOUBLE
s2n_z_autoSignal-to-noise of the detection within z_autoDOUBLE
s2n_z_petroSignal-to-noise of the detection within z_petroDOUBLE
s2ndetSignal-to-Noise on Detection Image (FLUX_AUTO/FLUXERR_AUTO)DOUBLE
stell_massStellar Mass for the First Peak (log10(M_sun))DOUBLE
tbBPZ most likely spectral type for the First PeakDOUBLE
thetaPosition Angle (CCW/x)DOUBLE
ujava_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
ujava_autoTotal-restricted magnitude [AB]DOUBLE
ujava_petroTotal magnitude [AB]DOUBLE
xX-pixel coordinateDOUBLE
yY-pixel coordinateDOUBLE
z_aperCircular-3arcsec-Diameter-Aperture magnitude [AB]DOUBLE
z_autoTotal-restricted magnitude [AB]DOUBLE
z_petroTotal magnitude [AB]DOUBLE
zbBPZ most likely redshift for the First PeakDOUBLE
zb_maxUpper limit (95p confidence) for the First PeakDOUBLE
zb_minLower limit (95p confidence) for the First PeakDOUBLE