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Table 8.

Contents of the OTELO multi-wavelength catalogue.

Parameter Description
idobj OTELO object number in raw catalogue
x, y Logical coordinates of the object in OTELO-Deep image
RA, Dec Equatorial coordinates (J2000.0) of the object in OTELO-Deep image
dmodelXa Magnitude from detection model-fitting in X-band of the core catalogue
edmodelX RMS error on detection model-fitting magnitude
isoareaX Isophotal area
fradiX-n source radius at n-per cent of flux, with n=20, 50, 80
spreadmX Spread parameter from model-fitting magnitude
espreadmX Spread parameter error from model-fitting magnitude
clasX SExtractor star/galaxy classifier output
iflagX SExtractor standard flag
totalZb Total magnitude in the Z-complementary catalogue
etotalZ Total magnitude error in the Z-complementary catalogue
els_preliminary ELS preliminary candidate flag
zspec Spectroscopic redshift from DEEP2 survey (Newman et al. 2013)
zp_reliable_T04 Most reliable photo-z from CFHTLS-T04 (Coupon et al. 2009)
zp_first_T04 Best photo-z estimate from CFHTLS-T04
zp_left_68_T04 Minimum photo-z from Δχ2 = 1.0 (68%) from CFHTLS-T04
zp_right_68_T04 Maximum photo-z from Δχ2 = 1.0 (68%) from CFHTLS-T04
z_BEST_deepQc Best galaxy model photo-z estimate
z_BEST68_LOW_deepQ Minimum photo-z from Δχ2 = 1.0 (68%)
z_BEST68_HIGH_deepQ Maximum photo-z from Δχ2 = 1.0 (68%)
CHI_BEST_deepQ Lowest χ2 for galaxy templates
MOD_BEST_deepQ Galaxy model for best CHI_BEST
EBV_BEST_deepQ Reddening colour excess E(B − V)
NBAND_USED_deepQ Number of bands used in photo-z fitting
z_SEC_deepQ Secondary photo-z solution
CHI_SEC_deepQ χ2 for secondary photo-z solution
MOD_SEC_deepQ Galaxy model for CHI_SEC
z_QSO_deepQ QSO model photo-z
CHI_QSO_deepQ χ2 for Z_QSO
MOD_QSO_deepQ Galaxy model for CHI_QSO
CHI_STAR_deepQ χ2 for MOD_STAR
MOD_STAR_deepQ Fitted star model
LUM_TIR_BEST_deepQ IR luminosity from MOD_FIR (when apply)
LIB_FIR_deepQ FIR library used (when apply)
MOD_FIR_deepQ FIR model fitted (when apply)
CHI_FIR_deepQ χ2 for FIR template fitting (when apply)

Notes.(a)Where X is D (OTELO-Deep), u, g, r, i, z (CFHT filters), HST-ACS606, HST-ACS814, J, H or Ks. (b)Where Z is Chandra, FUV or NUV from GALEX, 3.6, 4.5, 5.8, 8.0, or 24 μm from Spitzer, or 100, 160, 250, 300, 500 μm from Herschel. (c)Where Q is Y or N: including/not including OTELOInt data in photo-z solutions, respectively.

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