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Table: euclid_q1.phz_photo_z
(The bold columns are indexed columns)
Column NameDescriptionDatatype
alt_tom_bin_idThe identifier of the alternate tomographic bin the source belongs to (Equidistant-bins)INTEGER
best_chi2Chi2 of the best fit model or the closest neighborDOUBLE
bias_idThe identifier to be used for retrieving the bias correction shift from the bias correction mapINTEGER
flag_som_alt_tomobinFlag telling if the source belong to a combination of SOM cell and Alt Tom. bin which can be calibrated (=1) or not (=0).INTEGER
flag_som_pos_tomobinFlag telling if the source belong to a combination of SOM cell and POS Tom. bin which can be calibrated (=1) or not (=0).INTEGER
flag_som_tomobinFlag telling if the source belong to a combination of SOM cell and Tom. bin which can be calibrated (=1) or not (=0).INTEGER
flux_g_ext_decam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for g-ext DECamDOUBLE
flux_g_ext_hsc_unifUnified flux recomputed after correction from galactic extinction and filter shifts for g-ext HSCDOUBLE
flux_g_ext_lsst_unifUnified flux recomputed after correction from galactic extinction and filter shifts for g-ext LSSTDOUBLE
flux_h_unifUnified flux recomputed after correction from galactic extinction and filter shifts for H bandDOUBLE
flux_i_ext_decam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for i-ext DECamDOUBLE
flux_i_ext_lsst_unifUnified flux recomputed after correction from galactic extinction and filter shifts for i-ext LSSTDOUBLE
flux_i_ext_panstarrs_unifUnified flux recomputed after correction from galactic extinction and filter shifts for i-ext PanstarrsDOUBLE
flux_j_unifUnified flux recomputed after correction from galactic extinction and filter shifts for J bandDOUBLE
flux_r_ext_decam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for r-ext DECamDOUBLE
flux_r_ext_lsst_unifUnified flux recomputed after correction from galactic extinction and filter shifts for r-ext LSSTDOUBLE
flux_r_ext_megacam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for r-ext MegacamDOUBLE
flux_u_ext_decam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for u-ext DECamDOUBLE
flux_u_ext_lsst_unifUnified flux recomputed after correction from galactic extinction and filter shifts for u-ext LSSTDOUBLE
flux_u_ext_megacam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for u-ext MegacamDOUBLE
flux_vis_unifUnified flux recomputed after correction from galactic extinction and filter shifts for VIS bandDOUBLE
flux_y_unifUnified flux recomputed after correction from galactic extinction and filter shifts for Y bandDOUBLE
flux_z_ext_decam_unifUnified flux recomputed after correction from galactic extinction and filter shifts for z-ext DECamDOUBLE
flux_z_ext_hsc_unifUnified flux recomputed after correction from galactic extinction and filter shifts for z-ext HSCDOUBLE
flux_z_ext_lsst_unifUnified flux recomputed after correction from galactic extinction and filter shifts for z-ext LSSTDOUBLE
fluxerr_g_ext_decam_unifUnified flux error for g-ext DECam bandDOUBLE
fluxerr_g_ext_hsc_unifUnified flux error for g-ext HSC bandDOUBLE
fluxerr_g_ext_lsst_unifUnified flux error for g-ext LSST bandDOUBLE
fluxerr_h_unifUnified flux error for H bandDOUBLE
fluxerr_i_ext_decam_unifUnified flux error for i-ext DECam bandDOUBLE
fluxerr_i_ext_lsst_unifUnified flux error for i-ext LSST bandDOUBLE
fluxerr_i_ext_panstarrs_unifUnified flux error for i-ext Panstarrs bandDOUBLE
fluxerr_j_unifUnified flux error for J bandDOUBLE
fluxerr_r_ext_decam_unifUnified flux error for r-ext DECam bandDOUBLE
fluxerr_r_ext_lsst_unifUnified flux error for r-ext LSST bandDOUBLE
fluxerr_r_ext_megacam_unifUnified flux error for r-ext Megacam bandDOUBLE
fluxerr_u_ext_decam_unifUnified flux error for u-ext DECam bandDOUBLE
fluxerr_u_ext_lsst_unifUnified flux error for u-ext LSST bandDOUBLE
fluxerr_u_ext_megacam_unifUnified flux error for u-ext Megacam bandDOUBLE
fluxerr_vis_unifUnified flux error for VIS bandDOUBLE
fluxerr_y_unifUnified flux error for Y bandDOUBLE
fluxerr_z_ext_decam_unifUnified flux error for z-ext DECam bandDOUBLE
fluxerr_z_ext_hsc_unifUnified flux error for z-ext HSC bandDOUBLE
fluxerr_z_ext_lsst_unifUnified flux error for z-ext LSST bandDOUBLE
ie_cuts_weights_1Vector of probability to be a usable source for different VIS MAG cuts [20.25, 21.25, 22.25, 24.5]DOUBLE
ie_cuts_weights_2Vector of probability to be a usable source for different VIS MAG cuts [20.25, 21.25, 22.25, 24.5]DOUBLE
ie_cuts_weights_3Vector of probability to be a usable source for different VIS MAG cuts [20.25, 21.25, 22.25, 24.5]DOUBLE
ie_cuts_weights_4Vector of probability to be a usable source for different VIS MAG cuts [20.25, 21.25, 22.25, 24.5]DOUBLE
object_idUnique ID of the object in the survey, as set by MERBIGINT
photometric_systemEncode the Photometric band configuration (indicating also the number of missing columns)INTEGER
phz_70_int_1Lower bound of the smallest PHZ PDF interval containing 70% of the probabilityREAL
phz_70_int_2Upper bound of the smallest PHZ PDF interval containing 70% of the probabilityREAL
phz_90_int_1Lower bound of the smallest PHZ PDF interval containing 90% of the probabilityREAL
phz_90_int_2Upper bound of the smallest PHZ PDF interval containing 90% of the probabilityREAL
phz_95_int_1Lower bound of the smallest PHZ PDF interval containing 95% of the probabilityREAL
phz_95_int_2Upper bound of the smallest PHZ PDF interval containing 95% of the probabilityREAL
phz_classificationClassification flag: 1 if the source is accepted as star, 2 if it is accepted as a galaxy 4 if it is accepted as a QSO 8 if the source is accepted as a globular ClusterINTEGER
phz_flagsAn integer containing the flags of the PHZ processing. Meaning: 0 => OK, 1 => NNPZ flag: no close neighbor, 10 not VIS detected, 11 missing band, 12 too faintINTEGER
phz_medianThe median of the PHZ PDFREAL
phz_mode_1The first mode of the PHZ PDFREAL
phz_mode_1_areaThe total area of the first modeREAL
phz_mode_2The second mode of the PHZ PDFREAL
phz_mode_2_areaThe total area of the second modeREAL
phz_weightProbability to be a usable source at VIS MAG=23.5DOUBLE
pos_tom_bin_idThe identifier of the photometric clustering tomographic bin the source belongs to (Equipopulated-bins)INTEGER
random_idRandom ID in the range 0.0 => 100.0REAL
tom_bin_idThe identifier of the tomographic bin the source belongs to (Equipopulated-bins)INTEGER