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Table: des_dr1.y3_gold
(The bold columns are indexed columns)
| Column Name | Description | Datatype |
|---|---|---|
| a_fiducial_g | SED-independent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) in band GRIZY [magnitudes] | REAL |
| a_fiducial_i | SED-independent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) in band GRIZY [magnitudes] | REAL |
| a_fiducial_r | SED-independent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) in band GRIZY [magnitudes] | REAL |
| a_fiducial_y | SED-independent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) in band GRIZY [magnitudes] | REAL |
| a_fiducial_z | SED-independent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) in band GRIZY [magnitudes] | REAL |
| a_image | Detection image based basic shape parameter; A = semimajor-axis [pixels] | REAL |
| a_sed_lenz17_g | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Lenz et al. (2017) [magnitudes] | REAL |
| a_sed_lenz17_i | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Lenz et al. (2017) [magnitudes] | REAL |
| a_sed_lenz17_r | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Lenz et al. (2017) [magnitudes] | REAL |
| a_sed_lenz17_y | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Lenz et al. (2017) [magnitudes] | REAL |
| a_sed_lenz17_z | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Lenz et al. (2017) [magnitudes] | REAL |
| a_sed_planck13_g | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Planck Collaboration (2014) [magnitudes] | REAL |
| a_sed_planck13_i | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Planck Collaboration (2014) [magnitudes] | REAL |
| a_sed_planck13_r | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Planck Collaboration (2014) [magnitudes] | REAL |
| a_sed_planck13_y | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Planck Collaboration (2014) [magnitudes] | REAL |
| a_sed_planck13_z | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Planck Collaboration (2014) [magnitudes] | REAL |
| a_sed_sfd98_g | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) ; used in the CORRECTED columns; current recommendation [magnitudes] | REAL |
| a_sed_sfd98_i | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) ; used in the CORRECTED columns; current recommendation [magnitudes] | REAL |
| a_sed_sfd98_r | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) ; used in the CORRECTED columns; current recommendation [magnitudes] | REAL |
| a_sed_sfd98_y | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) ; used in the CORRECTED columns; current recommendation [magnitudes] | REAL |
| a_sed_sfd98_z | SED-dependent interstellar extinction based on the E(B - V) reddening maps from Schlegel, Finkbeiner & Davis (1998) ; used in the CORRECTED columns; current recommendation [magnitudes] | REAL |
| alphawin_j2000 | Right Ascension (J2000.0) of the object using a Gaussian window with a FWHM corresponding to the disk containing 50% of the flux. [degrees] | DOUBLE |
| b | Latitude in Galactic coordinates [degrees] | REAL |
| b_image | Detection image based basic shape parameter; B = semiminor-axis [pixels] | REAL |
| bpz_template_id_mof | Template identification from the BPZ code | INTEGER |
| bpz_template_id_sof | Template identification from the BPZ code | INTEGER |
| bpz_zmc_mof | MonteCarlo instance from the redshift distribution computed from BPZ | DOUBLE |
| bpz_zmc_sof | MonteCarlo instance from the redshift distribution computed from BPZ | DOUBLE |
| bpz_zmean_mof | Mean of the redshift distribution computed from BPZ | DOUBLE |
| bpz_zmean_sof | Mean of the redshift distribution computed from BPZ | DOUBLE |
| bpz_zmode_mof | Mode of the redshift distribution computed from BPZ | DOUBLE |
| bpz_zmode_sof | Mode of the redshift distribution computed from BPZ | DOUBLE |
| bpz_zsigma68_mof | Width of the 68% quantile | DOUBLE |
| bpz_zsigma68_sof | Width of the 68% quantile | DOUBLE |
| bpz_zsigma_mof | Width of the redshift distribution computed from BPZ | DOUBLE |
| bpz_zsigma_sof | Width of the redshift distribution computed from BPZ | DOUBLE |
| class_star_g | Morphology based star-galaxy classifier from SExtractor. Values between 0 (galaxies) and 1 (stars). | REAL |
| class_star_i | Morphology based star-galaxy classifier from SExtractor. Values between 0 (galaxies) and 1 (stars). | REAL |
| class_star_r | Morphology based star-galaxy classifier from SExtractor. Values between 0 (galaxies) and 1 (stars). | REAL |
| class_star_y | Morphology based star-galaxy classifier from SExtractor. Values between 0 (galaxies) and 1 (stars). | REAL |
| class_star_z | Morphology based star-galaxy classifier from SExtractor. Values between 0 (galaxies) and 1 (stars). | REAL |
| coadd_object_id | Unique identifier for the coadded objects | BIGINT |
| dec | Declination (J2000.0) with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed) [degrees] | DOUBLE |
| delta_mag_chrom_g | Coadd object chromatic correction using an appropriate spectral template for the object. See section 4.3 of Sevilla-Noarbe et al. (2021) | REAL |
| delta_mag_chrom_i | Coadd object chromatic correction using an appropriate spectral template for the object. See section 4.3 of Sevilla-Noarbe et al. (2021) | REAL |
| delta_mag_chrom_r | Coadd object chromatic correction using an appropriate spectral template for the object. See section 4.3 of Sevilla-Noarbe et al. (2021) | REAL |
| delta_mag_chrom_y | Coadd object chromatic correction using an appropriate spectral template for the object. See section 4.3 of Sevilla-Noarbe et al. (2021) | REAL |
| delta_mag_chrom_z | Coadd object chromatic correction using an appropriate spectral template for the object. See section 4.3 of Sevilla-Noarbe et al. (2021) | REAL |
| delta_mag_y4_g | Updates to photometry using Year 4 imaging. See section 4.3 of Sevilla-Noarbe et al. (2021). | REAL |
| delta_mag_y4_i | Updates to photometry using Year 4 imaging. See section 4.3 of Sevilla-Noarbe et al. (2021). | REAL |
| delta_mag_y4_r | Updates to photometry using Year 4 imaging. See section 4.3 of Sevilla-Noarbe et al. (2021). | REAL |
| delta_mag_y4_y | Updates to photometry using Year 4 imaging. See section 4.3 of Sevilla-Noarbe et al. (2021). | REAL |
| delta_mag_y4_z | Updates to photometry using Year 4 imaging. See section 4.3 of Sevilla-Noarbe et al. (2021). | REAL |
| deltawin_j2000 | Declination (J2000.0) of the object using a Gaussian window with a FWHM corresponding to the disk containing 50% of the flux. [degrees] | DOUBLE |
| dnf_zmc_mof | Nearest neighbor redshift from the reference set produced by the DNF photo-z estimator. Appropriate for building ensemble redshift distributions | REAL |
| dnf_zmc_sof | Nearest neighbor redshift from the reference set produced by the DNF photo-z estimator. Appropriate for building ensemble redshift distributions | REAL |
| dnf_zmean_mof | Best redshift estimate from the DNF photo-z algorithm. | REAL |
| dnf_zmean_sof | Best redshift estimate from the DNF photo-z algorithm. | REAL |
| dnf_zsigma_mof | Error estimate in redshift from the DNF photo-z algorithm. | REAL |
| dnf_zsigma_sof | Error estimate in redshift from the DNF photo-z algorithm. | REAL |
| ebv_lenz17 | E(B-V) reddening coefficient from Lenz et al. (2017) | REAL |
| ebv_planck13 | E(B-V) reddening coefficient from Planck Collaboration (2014) | REAL |
| ebv_sfd98 | E(B-V) reddening coefficient from Schlegel, Finkbeiner & Davis (1998) | REAL |
| elat | Ecliptic Latitude | DOUBLE |
| elon | Ecliptic Longitude | DOUBLE |
| erra_image | Uncertainty in major axis size, from isophotal model [pixel] | DOUBLE |
| errb_image | Uncertainty in minor axis size, from isophotal model [pixel] | REAL |
| errtheta_image | Uncertainty in source position, from isophotal model [degrees] | REAL |
| extended_class_coadd | Star/galaxy separation using SExtractor photometry and SPREAD_MODEL, SPREAD_MODEL_ERR in the i band. 0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: No data | SMALLINT |
| extended_class_mash_mof | Star/galaxy separation using MOF/SOF photometry in the i band, and WAVG and finally coadd quantities in case of missing values. 0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: No data | SMALLINT |
| extended_class_mash_sof | Star/galaxy separation using MOF/SOF photometry in the i band, and WAVG and finally coadd quantities in case of missing values. 0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: No data | SMALLINT |
| extended_class_mof | Star/galaxy separation using MOF/SOF photometry and T_SIZE in the i band. 0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: No data | SMALLINT |
| extended_class_sof | Star/galaxy separation using MOF/SOF photometry and T_SIZE in the i band. 0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: No data | SMALLINT |
| extended_class_wavg | Star/galaxy separation using WAVG photometry and SPREAD_MODEL, SPREAD_MODEL_ERR in the i band. 0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: No data | SMALLINT |
| flags_badregions | Flag describing whether the object is contained in a region with potentially problematic processing. See Sevilla-Noarbe et al. (2021) for description. | INTEGER |
| flags_footprint | Flag describing whether the object is contained in the fiducial footprint of the survey. See Sevilla-Noarbe et al. (2021) for description. | INTEGER |
| flags_foreground | Flag describing whether the object is contained in a region with a foreground astrophysical object. See Sevilla-Noarbe et al. (2021) for description. | INTEGER |
| flags_gold | Flag describing object anomalies. See Sevilla-Noarbe et al. (2021) for description. | INTEGER |
| flux_aper_8_g | Flux measurement in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_aper_8_i | Flux measurement in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_aper_8_r | Flux measurement in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_aper_8_y | Flux measurement in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_aper_8_z | Flux measurement in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_auto_g | Flux measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_auto_i | Flux measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_auto_r | Flux measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_auto_y | Flux measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_auto_z | Flux measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius; MAG=30-2.5*log10(FLUX) [ADU] | REAL |
| flux_detmodel_g | Flux measurement, for a bulge + disk model fit on the detection image [ADU] | REAL |
| flux_detmodel_i | Flux measurement, for a bulge + disk model fit on the detection image [ADU] | REAL |
| flux_detmodel_r | Flux measurement, for a bulge + disk model fit on the detection image [ADU] | REAL |
| flux_detmodel_y | Flux measurement, for a bulge + disk model fit on the detection image [ADU] | REAL |
| flux_detmodel_z | Flux measurement, for a bulge + disk model fit on the detection image [ADU] | REAL |
| flux_radius_g | Half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel] | REAL |
| flux_radius_i | Half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel] | REAL |
| flux_radius_r | Half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel] | REAL |
| flux_radius_y | Half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel] | REAL |
| flux_radius_z | Half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel] | REAL |
| fluxerr_aper_8_g | RMS error estimate of FLUX_APER_8 [ADU] | REAL |
| fluxerr_aper_8_i | RMS error estimate of FLUX_APER_8 [ADU] | REAL |
| fluxerr_aper_8_r | RMS error estimate of FLUX_APER_8 [ADU] | REAL |
| fluxerr_aper_8_y | RMS error estimate of FLUX_APER_8 [ADU] | REAL |
| fluxerr_aper_8_z | RMS error estimate of FLUX_APER_8 [ADU] | REAL |
| fluxerr_auto_g | RMS error estimate of FLUX_AUTO [ADU] | REAL |
| fluxerr_auto_i | RMS error estimate of FLUX_AUTO [ADU] | REAL |
| fluxerr_auto_r | RMS error estimate of FLUX_AUTO [ADU] | REAL |
| fluxerr_auto_y | RMS error estimate of FLUX_AUTO [ADU] | REAL |
| fluxerr_auto_z | RMS error estimate of FLUX_AUTO [ADU] | REAL |
| fluxerr_detmodel_g | RMS error estimate of FLUX_DETMODEL measurement [ADU] | REAL |
| fluxerr_detmodel_i | RMS error estimate of FLUX_DETMODEL measurement [ADU] | REAL |
| fluxerr_detmodel_r | RMS error estimate of FLUX_DETMODEL measurement [ADU] | REAL |
| fluxerr_detmodel_y | RMS error estimate of FLUX_DETMODEL measurement [ADU] | REAL |
| fluxerr_detmodel_z | RMS error estimate of FLUX_DETMODEL measurement [ADU] | REAL |
| frac_det_griz | Fractional area of Healpix pixel covered simultaneously by griz bands | REAL |
| frac_det_grizy | Fractional area of Healpix pixel covered simultaneously by grizY bands | REAL |
| hpix_16384 | Healpix index for NSIDE = 16384 in NEST schema for the object | BIGINT |
| hpix_4096 | Healpix index for NSIDE = 4096 in NEST schema for the object | BIGINT |
| htm9 | Ninth level (~10 arcmin resolution) Hierarchical Triangular Mesh index (Szalay et al. 2007) | INTEGER |
| imaflags_iso_g | Flag identifying sources with missing/flagged pixels, considering all single epoch images | INTEGER |
| imaflags_iso_i | Flag identifying sources with missing/flagged pixels, considering all single epoch images | INTEGER |
| imaflags_iso_r | Flag identifying sources with missing/flagged pixels, considering all single epoch images | INTEGER |
| imaflags_iso_y | Flag identifying sources with missing/flagged pixels, considering all single epoch images | INTEGER |
| imaflags_iso_z | Flag identifying sources with missing/flagged pixels, considering all single epoch images | INTEGER |
| kron_radius | Detection image luminosity weighted radius for the object, encompassing approximately 90% of the total flux | REAL |
| l | Longitude in Galactic coordinates [degrees] | REAL |
| mag_aper_8_g | Magnitude measured in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter [magnitudes] | REAL |
| mag_aper_8_i | Magnitude measured in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter [magnitudes] | REAL |
| mag_aper_8_r | Magnitude measured in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter [magnitudes] | REAL |
| mag_aper_8_y | Magnitude measured in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter [magnitudes] | REAL |
| mag_aper_8_z | Magnitude measured in a circular aperture of 22.22 pixels (5.8437 arcsecs) diameter [magnitudes] | REAL |
| mag_auto_g | Magnitude measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius [magnitudes] | REAL |
| mag_auto_i | Magnitude measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius [magnitudes] | REAL |
| mag_auto_r | Magnitude measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius [magnitudes] | REAL |
| mag_auto_y | Magnitude measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius [magnitudes] | REAL |
| mag_auto_z | Magnitude measurement in an elliptical aperture, shaped by the second moments of the object and scaled by the Kron radius [magnitudes] | REAL |
| mag_detmodel_g | Magnitude measurement, for a bulge + disk model fit on the detection image [magnitudes] | REAL |
| mag_detmodel_i | Magnitude measurement, for a bulge + disk model fit on the detection image [magnitudes] | REAL |
| mag_detmodel_r | Magnitude measurement, for a bulge + disk model fit on the detection image [magnitudes] | REAL |
| mag_detmodel_y | Magnitude measurement, for a bulge + disk model fit on the detection image [magnitudes] | REAL |
| mag_detmodel_z | Magnitude measurement, for a bulge + disk model fit on the detection image [magnitudes] | REAL |
| mag_psf_g | Magnitude measured using the coadd PSF (use caution as this PSF varies discontinuously across footprint) [magnitudes] | REAL |
| mag_psf_i | Magnitude measured using the coadd PSF (use caution as this PSF varies discontinuously across footprint) [magnitudes] | REAL |
| mag_psf_r | Magnitude measured using the coadd PSF (use caution as this PSF varies discontinuously across footprint) [magnitudes] | REAL |
| mag_psf_y | Magnitude measured using the coadd PSF (use caution as this PSF varies discontinuously across footprint) [magnitudes] | REAL |
| mag_psf_z | Magnitude measured using the coadd PSF (use caution as this PSF varies discontinuously across footprint) [magnitudes] | REAL |
| magerr_aper_8_g | Error in MAG_APER_8, scaled from FLUXERR_APER_8 [magnitudes] | REAL |
| magerr_aper_8_i | Error in MAG_APER_8, scaled from FLUXERR_APER_8 [magnitudes] | REAL |
| magerr_aper_8_r | Error in MAG_APER_8, scaled from FLUXERR_APER_8 [magnitudes] | REAL |
| magerr_aper_8_y | Error in MAG_APER_8, scaled from FLUXERR_APER_8 [magnitudes] | REAL |
| magerr_aper_8_z | Error in MAG_APER_8, scaled from FLUXERR_APER_8 [magnitudes] | REAL |
| magerr_auto_g | Error in MAG_AUTO, scaled from FLUXERR_AUTO [magnitudes] | REAL |
| magerr_auto_i | Error in MAG_AUTO, scaled from FLUXERR_AUTO [magnitudes] | REAL |
| magerr_auto_r | Error in MAG_AUTO, scaled from FLUXERR_AUTO [magnitudes] | REAL |
| magerr_auto_y | Error in MAG_AUTO, scaled from FLUXERR_AUTO [magnitudes] | REAL |
| magerr_auto_z | Error in MAG_AUTO, scaled from FLUXERR_AUTO [magnitudes] | REAL |
| magerr_detmodel_g | Error in MAG_DETMODEL, scaled from FLUXERR_DETMODEL [magnitudes] | REAL |
| magerr_detmodel_i | Error in MAG_DETMODEL, scaled from FLUXERR_DETMODEL [magnitudes] | REAL |
| magerr_detmodel_r | Error in MAG_DETMODEL, scaled from FLUXERR_DETMODEL [magnitudes] | REAL |
| magerr_detmodel_y | Error in MAG_DETMODEL, scaled from FLUXERR_DETMODEL [magnitudes] | REAL |
| magerr_detmodel_z | Error in MAG_DETMODEL, scaled from FLUXERR_DETMODEL [magnitudes] | REAL |
| magerr_psf_g | Error in MAG_PSF, scaled from MAG_PSF [magnitudes] | REAL |
| magerr_psf_i | Error in MAG_PSF, scaled from MAG_PSF [magnitudes] | REAL |
| magerr_psf_r | Error in MAG_PSF, scaled from MAG_PSF [magnitudes] | REAL |
| magerr_psf_y | Error in MAG_PSF, scaled from MAG_PSF [magnitudes] | REAL |
| magerr_psf_z | Error in MAG_PSF, scaled from MAG_PSF [magnitudes] | REAL |
| mof_cm_chi2per | Chi2 per degree of freedom of the composite model fit | DOUBLE |
| mof_cm_dof | Number of the degrees of freedom for the composite model fit | DOUBLE |
| mof_cm_flux_cov_g_g | Diagonal covariance of the MOF CM flux in the g band | DOUBLE |
| mof_cm_flux_cov_i_i | Diagonal covariance of the MOF CM flux in the i band | DOUBLE |
| mof_cm_flux_cov_r_r | Diagonal covariance of the MOF CM flux in the r band | DOUBLE |
| mof_cm_flux_cov_z_z | Diagonal covariance of the MOF CM flux in the z band | DOUBLE |
| mof_cm_flux_g | Measured MOF composite model flux [ADU] | DOUBLE |
| mof_cm_flux_i | Measured MOF composite model flux [ADU] | DOUBLE |
| mof_cm_flux_r | Measured MOF composite model flux [ADU] | DOUBLE |
| mof_cm_flux_s2n_g | MOF composite model flux signal to noise ratio | DOUBLE |
| mof_cm_flux_s2n_i | MOF composite model flux signal to noise ratio | DOUBLE |
| mof_cm_flux_s2n_r | MOF composite model flux signal to noise ratio | DOUBLE |
| mof_cm_flux_s2n_z | MOF composite model flux signal to noise ratio | DOUBLE |
| mof_cm_flux_z | Measured MOF composite model flux [ADU] | DOUBLE |
| mof_cm_fracdev | MOF composite model fraction of de Vaucouleurs flux: cm = fracdev * devaucouleurs + (1-fracdev) * exponential | DOUBLE |
| mof_cm_fracdev_err | Error in FRACDEV | DOUBLE |
| mof_cm_fracdev_noclip | Value of FRACDEV if not clipped to [0,1] range | DOUBLE |
| mof_cm_g_1 | MOF based shape component 1 (reduced version of e1) | DOUBLE |
| mof_cm_g_2 | MOF based shape component 2 (reduced version of e2) | DOUBLE |
| mof_cm_g_cov_1_1 | MOF based shape covariance component 1-1 | DOUBLE |
| mof_cm_g_cov_1_2 | MOF based shape covariance component 1-2 | DOUBLE |
| mof_cm_g_cov_2_1 | MOF based shape covariance component 2-1 | DOUBLE |
| mof_cm_g_cov_2_2 | MOF based shape covariance component 2-2 | DOUBLE |
| mof_cm_logsb_g | Logarithm of the MOF based surface brightness | DOUBLE |
| mof_cm_logsb_i | Logarithm of the MOF based surface brightness | DOUBLE |
| mof_cm_logsb_r | Logarithm of the MOF based surface brightness | DOUBLE |
| mof_cm_logsb_z | Logarithm of the MOF based surface brightness | DOUBLE |
| mof_cm_mag_corrected_g | MOF corrected magnitude = MOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| mof_cm_mag_corrected_i | MOF corrected magnitude = MOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| mof_cm_mag_corrected_r | MOF corrected magnitude = MOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| mof_cm_mag_corrected_z | MOF corrected magnitude = MOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| mof_cm_mag_err_g | Uncertainty in MOF magnitude | DOUBLE |
| mof_cm_mag_err_i | Uncertainty in MOF magnitude | DOUBLE |
| mof_cm_mag_err_r | Uncertainty in MOF magnitude | DOUBLE |
| mof_cm_mag_err_z | Uncertainty in MOF magnitude | DOUBLE |
| mof_cm_mag_g | Magnitude from MOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_cm_mag_i | Magnitude from MOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_cm_mag_r | Magnitude from MOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_cm_mag_z | Magnitude from MOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_cm_t | Size squared of the object: T=+ [arcsec**2] | DOUBLE |
| mof_cm_t_err | Error in size squared [arcsec**2] | DOUBLE |
| mof_cm_tdbyte | Ratio of sizes Tdev/Texp | DOUBLE |
| mof_flags | Overall image processing flags. Can contain NULLs for objects with unfinished processing for MOF | BIGINT |
| mof_psf_flux_err_g | Uncertainty in measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_err_i | Uncertainty in measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_err_r | Uncertainty in measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_err_z | Uncertainty in measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_g | Measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_i | Measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_r | Measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_flux_s2n_g | MOF PSF flux signal to noise ratio | DOUBLE |
| mof_psf_flux_s2n_i | MOF PSF flux signal to noise ratio | DOUBLE |
| mof_psf_flux_s2n_r | MOF PSF flux signal to noise ratio | DOUBLE |
| mof_psf_flux_s2n_z | MOF PSF flux signal to noise ratio | DOUBLE |
| mof_psf_flux_z | Measured MOF PSF flux [ADU] | DOUBLE |
| mof_psf_mag_err_g | Uncertainty in MOF PSF magnitude | DOUBLE |
| mof_psf_mag_err_i | Uncertainty in MOF PSF magnitude | DOUBLE |
| mof_psf_mag_err_r | Uncertainty in MOF PSF magnitude | DOUBLE |
| mof_psf_mag_err_z | Uncertainty in MOF PSF magnitude | DOUBLE |
| mof_psf_mag_g | Magnitude from MOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_psf_mag_i | Magnitude from MOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_psf_mag_r | Magnitude from MOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mof_psf_mag_z | Magnitude from MOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| mu_eff_model_g | Effective model surface brightness above background. The surface brightness is measured at the isophote which includes half of the flux of the model, above background [mag./sq.arcsec] | REAL |
| mu_eff_model_i | Effective model surface brightness above background. The surface brightness is measured at the isophote which includes half of the flux of the model, above background [mag./sq.arcsec] | REAL |
| mu_eff_model_r | Effective model surface brightness above background. The surface brightness is measured at the isophote which includes half of the flux of the model, above background [mag./sq.arcsec] | REAL |
| mu_eff_model_y | Effective model surface brightness above background. The surface brightness is measured at the isophote which includes half of the flux of the model, above background [mag./sq.arcsec] | REAL |
| mu_eff_model_z | Effective model surface brightness above background. The surface brightness is measured at the isophote which includes half of the flux of the model, above background [mag./sq.arcsec] | REAL |
| mu_max_g | Surface brightness at the brightest pixel [mag./sq.arcsec] | REAL |
| mu_max_i | Surface brightness at the brightest pixel [mag./sq.arcsec] | REAL |
| mu_max_model_g | Maximum surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_max_model_i | Maximum surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_max_model_r | Maximum surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_max_model_y | Maximum surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_max_model_z | Maximum surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_max_r | Surface brightness at the brightest pixel [mag./sq.arcsec] | REAL |
| mu_max_y | Surface brightness at the brightest pixel [mag./sq.arcsec] | REAL |
| mu_max_z | Surface brightness at the brightest pixel [mag./sq.arcsec] | REAL |
| mu_mean_model_g | Mean surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_mean_model_i | Mean surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_mean_model_r | Mean surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_mean_model_y | Mean surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_mean_model_z | Mean surface brightness using the whole area inside the isophote used for MU_EFF_MODEL [mag./sq.arcsec] | REAL |
| mu_threshold_g | Surface brightness threshold (SExtractor parameter) [mag./sq.arcsec.] | REAL |
| mu_threshold_i | Surface brightness threshold (SExtractor parameter) [mag./sq.arcsec.] | REAL |
| mu_threshold_r | Surface brightness threshold (SExtractor parameter) [mag./sq.arcsec.] | REAL |
| mu_threshold_y | Surface brightness threshold (SExtractor parameter) [mag./sq.arcsec.] | REAL |
| mu_threshold_z | Surface brightness threshold (SExtractor parameter) [mag./sq.arcsec.] | REAL |
| n_images_g | Number of (grizY) band exposures at the object location (from the Healpix map) | INTEGER |
| n_images_i | Number of (grizY) band exposures at the object location (from the Healpix map) | INTEGER |
| n_images_r | Number of (grizY) band exposures at the object location (from the Healpix map) | INTEGER |
| n_images_y | Number of (grizY) band exposures at the object location (from the Healpix map) | INTEGER |
| n_images_z | Number of (grizY) band exposures at the object location (from the Healpix map) | INTEGER |
| nepochs_g | Number of epochs the source is detected in single epoch images | INTEGER |
| nepochs_i | Number of epochs the source is detected in single epoch images | INTEGER |
| nepochs_r | Number of epochs the source is detected in single epoch images | INTEGER |
| nepochs_y | Number of epochs the source is detected in single epoch images | INTEGER |
| nepochs_z | Number of epochs the source is detected in single epoch images | INTEGER |
| niter_model_g | Number of iterations for convergence in SExtractor model fitting | INTEGER |
| niter_model_i | Number of iterations for convergence in SExtractor model fitting | INTEGER |
| niter_model_r | Number of iterations for convergence in SExtractor model fitting | INTEGER |
| niter_model_y | Number of iterations for convergence in SExtractor model fitting | INTEGER |
| niter_model_z | Number of iterations for convergence in SExtractor model fitting | INTEGER |
| object_number | SExtractor unique number for a processing tile | INTEGER |
| parent_number | SExtractor OBJECT_NUMBER of parent object of which this object is a deblended child | INTEGER |
| ra | Right Ascension (J2000.0) with quantized precision for indexing (ALPHAWIN_J2000 has full precision but not indexed) [degrees] | DOUBLE |
| random_id | Random ID in the range 0.0 => 100.0 | REAL |
| ring256 | Ring-scheme HEALPix (Gorski et al. 2005) index with NSIDE=256 (~14 arcmin resolution) | INTEGER |
| sextractor_flags_g | SExtractor 16-bit flag parameter which contains basic warnings about the source extraction process | SMALLINT |
| sextractor_flags_i | SExtractor 16-bit flag parameter which contains basic warnings about the source extraction process | SMALLINT |
| sextractor_flags_r | SExtractor 16-bit flag parameter which contains basic warnings about the source extraction process | SMALLINT |
| sextractor_flags_y | SExtractor 16-bit flag parameter which contains basic warnings about the source extraction process | SMALLINT |
| sextractor_flags_z | SExtractor 16-bit flag parameter which contains basic warnings about the source extraction process | SMALLINT |
| sof_cm_chi2per | Chi2 per degree of freedom of the composite model fit | DOUBLE |
| sof_cm_dof | Number of the degrees of freedom for the composite model fit | DOUBLE |
| sof_cm_flux_cov_g_g | Diagonal covariance of the SOF CM flux in the g band | DOUBLE |
| sof_cm_flux_cov_i_i | Diagonal covariance of the SOF CM flux in the i band | DOUBLE |
| sof_cm_flux_cov_r_r | Diagonal covariance of the SOF CM flux in the r band | DOUBLE |
| sof_cm_flux_cov_z_z | Diagonal covariance of the SOF CM flux in the z band | DOUBLE |
| sof_cm_flux_g | Measured SOF composite model flux [ADU] | DOUBLE |
| sof_cm_flux_i | Measured SOF composite model flux [ADU] | DOUBLE |
| sof_cm_flux_r | Measured SOF composite model flux [ADU] | DOUBLE |
| sof_cm_flux_s2n_g | SOF composite model flux signal to noise ratio | DOUBLE |
| sof_cm_flux_s2n_i | SOF composite model flux signal to noise ratio | DOUBLE |
| sof_cm_flux_s2n_r | SOF composite model flux signal to noise ratio | DOUBLE |
| sof_cm_flux_s2n_z | SOF composite model flux signal to noise ratio | DOUBLE |
| sof_cm_flux_z | Measured SOF composite model flux [ADU] | DOUBLE |
| sof_cm_fracdev | SOF composite model fraction of de Vaucouleurs flux: cm = fracdev * devaucouleurs + (1-fracdev) * exponential | REAL |
| sof_cm_fracdev_err | Error in FRACDEV | REAL |
| sof_cm_fracdev_noclip | Value of FRACDEV if not clipped to [0,1] range | REAL |
| sof_cm_g_1 | SOF based shape component 1 (reduced version of e1) | DOUBLE |
| sof_cm_g_2 | SOF based shape component 2 (reduced version of e2) | DOUBLE |
| sof_cm_g_cov_1_1 | SOF based shape covariance component 1-1 | DOUBLE |
| sof_cm_g_cov_1_2 | SOF based shape covariance component 1-2 | DOUBLE |
| sof_cm_g_cov_2_1 | SOF based shape covariance component 2-1 | DOUBLE |
| sof_cm_g_cov_2_2 | SOF based shape covariance component 2-2 | DOUBLE |
| sof_cm_logsb_g | Logarithm of the SOF based surface brightness | DOUBLE |
| sof_cm_logsb_i | Logarithm of the SOF based surface brightness | DOUBLE |
| sof_cm_logsb_r | Logarithm of the SOF based surface brightness | DOUBLE |
| sof_cm_logsb_z | Logarithm of the SOF based surface brightness | DOUBLE |
| sof_cm_mag_corrected_g | SOF corrected magnitude = SOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| sof_cm_mag_corrected_i | SOF corrected magnitude = SOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| sof_cm_mag_corrected_r | SOF corrected magnitude = SOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| sof_cm_mag_corrected_z | SOF corrected magnitude = SOF_CM_MAG + DELTA_MAG_Y4 + DELTA_MAG_CHROM + A_SED_SFD98 | DOUBLE |
| sof_cm_mag_err_g | Uncertainty in SOF magnitude | DOUBLE |
| sof_cm_mag_err_i | Uncertainty in SOF magnitude | DOUBLE |
| sof_cm_mag_err_r | Uncertainty in SOF magnitude | DOUBLE |
| sof_cm_mag_err_z | Uncertainty in SOF magnitude | DOUBLE |
| sof_cm_mag_g | Magnitude from SOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_cm_mag_i | Magnitude from SOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_cm_mag_r | Magnitude from SOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_cm_mag_z | Magnitude from SOF_CM_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_cm_t | Size squared of the object: T=+ [arcsec**2] | DOUBLE |
| sof_cm_t_err | Error in size squared [arcsec**2] | DOUBLE |
| sof_cm_tdbyte | Ratio of sizes Tdev/Texp | REAL |
| sof_flags | Overall image processing flags. Can contain NULLs for objects with unfinished processing for SOF | BIGINT |
| sof_psf_flux_err_g | Uncertainty in measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_err_i | Uncertainty in measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_err_r | Uncertainty in measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_err_z | Uncertainty in measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_g | Measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_i | Measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_r | Measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_flux_s2n_g | SOF PSF flux signal to noise ratio | DOUBLE |
| sof_psf_flux_s2n_i | SOF PSF flux signal to noise ratio | DOUBLE |
| sof_psf_flux_s2n_r | SOF PSF flux signal to noise ratio | DOUBLE |
| sof_psf_flux_s2n_z | SOF PSF flux signal to noise ratio | DOUBLE |
| sof_psf_flux_z | Measured SOF PSF flux [ADU] | DOUBLE |
| sof_psf_mag_err_g | Uncertainty in SOF PSF magnitude | DOUBLE |
| sof_psf_mag_err_i | Uncertainty in SOF PSF magnitude | DOUBLE |
| sof_psf_mag_err_r | Uncertainty in SOF PSF magnitude | DOUBLE |
| sof_psf_mag_err_z | Uncertainty in SOF PSF magnitude | DOUBLE |
| sof_psf_mag_g | Magnitude from SOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_psf_mag_i | Magnitude from SOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_psf_mag_r | Magnitude from SOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| sof_psf_mag_z | Magnitude from SOF_PSF_FLUX. MAG = 30-2.5*log10(FLUX) | DOUBLE |
| spread_model_g | Morphology based classifier based on a linear discriminant between the pixel map of the object convolved with the PSF model and the pixel map convolved with a PSF+exponential model. Values closer to 0 correspond to stars, larger values correspond to galaxies | REAL |
| spread_model_i | Morphology based classifier based on a linear discriminant between the pixel map of the object convolved with the PSF model and the pixel map convolved with a PSF+exponential model. Values closer to 0 correspond to stars, larger values correspond to galaxies | REAL |
| spread_model_r | Morphology based classifier based on a linear discriminant between the pixel map of the object convolved with the PSF model and the pixel map convolved with a PSF+exponential model. Values closer to 0 correspond to stars, larger values correspond to galaxies | REAL |
| spread_model_y | Morphology based classifier based on a linear discriminant between the pixel map of the object convolved with the PSF model and the pixel map convolved with a PSF+exponential model. Values closer to 0 correspond to stars, larger values correspond to galaxies | REAL |
| spread_model_z | Morphology based classifier based on a linear discriminant between the pixel map of the object convolved with the PSF model and the pixel map convolved with a PSF+exponential model. Values closer to 0 correspond to stars, larger values correspond to galaxies | REAL |
| spreaderr_model_g | Uncertainty in SPREAD_MODEL. | REAL |
| spreaderr_model_i | Uncertainty in SPREAD_MODEL. | REAL |
| spreaderr_model_r | Uncertainty in SPREAD_MODEL. | REAL |
| spreaderr_model_y | Uncertainty in SPREAD_MODEL. | REAL |
| spreaderr_model_z | Uncertainty in SPREAD_MODEL. | REAL |
| theta_j2000 | Position angle of the ellipse fit to the object with the N/S/E/W axes in equatorial J2000 coordinates, from non-windowed measurement. THETA_J2000 = THETA_IMAGE-90(MOD 180) [degrees] | REAL |
| tilename | Identifier of each one of the tiles on which the survey is gridded for data processing | VARCHAR |
| wavg_flux_psf_g | PSF flux using the weighted averaged values of single epoch objects (according to weight maps). Not valid if NEPOCHS = 0 [ADU] | REAL |
| wavg_flux_psf_i | PSF flux using the weighted averaged values of single epoch objects (according to weight maps). Not valid if NEPOCHS = 0 [ADU] | REAL |
| wavg_flux_psf_r | PSF flux using the weighted averaged values of single epoch objects (according to weight maps). Not valid if NEPOCHS = 0 [ADU] | REAL |
| wavg_flux_psf_y | PSF flux using the weighted averaged values of single epoch objects (according to weight maps). Not valid if NEPOCHS = 0 [ADU] | REAL |
| wavg_flux_psf_z | PSF flux using the weighted averaged values of single epoch objects (according to weight maps). Not valid if NEPOCHS = 0 [ADU] | REAL |
| wavg_fluxerr_psf_g | RMS error estimate of WAVG_FLUX_PSF [ADU] | REAL |
| wavg_fluxerr_psf_i | RMS error estimate of WAVG_FLUX_PSF [ADU] | REAL |
| wavg_fluxerr_psf_r | RMS error estimate of WAVG_FLUX_PSF [ADU] | REAL |
| wavg_fluxerr_psf_y | RMS error estimate of WAVG_FLUX_PSF [ADU] | REAL |
| wavg_fluxerr_psf_z | RMS error estimate of WAVG_FLUX_PSF [ADU] | REAL |
| wavg_mag_psf_g | Magnitude corresponding to MAG = 30-2.5*log10(WAVG_FLUX_PSF) [magnitudes] | REAL |
| wavg_mag_psf_i | Magnitude corresponding to MAG = 30-2.5*log10(WAVG_FLUX_PSF) [magnitudes] | REAL |
| wavg_mag_psf_r | Magnitude corresponding to MAG = 30-2.5*log10(WAVG_FLUX_PSF) [magnitudes] | REAL |
| wavg_mag_psf_y | Magnitude corresponding to MAG = 30-2.5*log10(WAVG_FLUX_PSF) [magnitudes] | REAL |
| wavg_mag_psf_z | Magnitude corresponding to MAG = 30-2.5*log10(WAVG_FLUX_PSF) [magnitudes] | REAL |
| wavg_magerr_psf_g | Uncertainty of WAVG_MAG_PSF, scaled from WAVG_FLUXERR_PSF [magnitudes] | REAL |
| wavg_magerr_psf_i | Uncertainty of WAVG_MAG_PSF, scaled from WAVG_FLUXERR_PSF [magnitudes] | REAL |
| wavg_magerr_psf_r | Uncertainty of WAVG_MAG_PSF, scaled from WAVG_FLUXERR_PSF [magnitudes] | REAL |
| wavg_magerr_psf_y | Uncertainty of WAVG_MAG_PSF, scaled from WAVG_FLUXERR_PSF [magnitudes] | REAL |
| wavg_magerr_psf_z | Uncertainty of WAVG_MAG_PSF, scaled from WAVG_FLUXERR_PSF [magnitudes] | REAL |
| wavg_spread_model_g | SPREAD MODEL using the weighted averaged values from single epoch detections | REAL |
| wavg_spread_model_i | SPREAD MODEL using the weighted averaged values from single epoch detections | REAL |
| wavg_spread_model_r | SPREAD MODEL using the weighted averaged values from single epoch detections | REAL |
| wavg_spread_model_y | SPREAD MODEL using the weighted averaged values from single epoch detections | REAL |
| wavg_spread_model_z | SPREAD MODEL using the weighted averaged values from single epoch detections | REAL |
| wavg_spreaderr_model_g | Uncertainty in WAVG_SPREAD_MODEL | REAL |
| wavg_spreaderr_model_i | Uncertainty in WAVG_SPREAD_MODEL | REAL |
| wavg_spreaderr_model_r | Uncertainty in WAVG_SPREAD_MODEL | REAL |
| wavg_spreaderr_model_y | Uncertainty in WAVG_SPREAD_MODEL | REAL |
| wavg_spreaderr_model_z | Uncertainty in WAVG_SPREAD_MODEL | REAL |
| xwin_image | X position of the barycenter of the object within the image using a Gaussian window with a FWHM corresponding to the radius of the aperture containing 50% of the flux [pixel] | DOUBLE |
| ywin_image | Y position of the barycenter of the object within the image using a Gaussian window with a FWHM corresponding to the radius of the aperture containing 50% of the flux [pixel] | DOUBLE |
