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Table: des_dr1.y3_gold_surveyconditions
(The bold columns are indexed columns)
Column NameDescriptionDatatype
airmass_max_gSecant of the max zenith anglereal
airmass_max_iSecant of the max zenith anglereal
airmass_max_rSecant of the max zenith anglereal
airmass_max_ySecant of the max zenith anglereal
airmass_max_zSecant of the max zenith anglereal
airmass_min_gSecant of the min zenith anglereal
airmass_min_iSecant of the min zenith anglereal
airmass_min_rSecant of the min zenith anglereal
airmass_min_ySecant of the min zenith anglereal
airmass_min_zSecant of the min zenith anglereal
airmass_wmean_gSecant of the mean zenith anglereal
airmass_wmean_iSecant of the mean zenith anglereal
airmass_wmean_rSecant of the mean zenith anglereal
airmass_wmean_ySecant of the mean zenith anglereal
airmass_wmean_zSecant of the mean zenith anglereal
depth_auto_gEstimate of the depth using MAG_AUTO photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_auto_iEstimate of the depth using MAG_AUTO photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_auto_rEstimate of the depth using MAG_AUTO photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_auto_yEstimate of the depth using MAG_AUTO photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_auto_zEstimate of the depth using MAG_AUTO photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_mof_gEstimate of the depth using MAG_MOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_mof_iEstimate of the depth using MAG_MOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_mof_rEstimate of the depth using MAG_MOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_mof_zEstimate of the depth using MAG_MOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_sof_gEstimate of the depth using MAG_SOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_sof_iEstimate of the depth using MAG_SOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_sof_rEstimate of the depth using MAG_SOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
depth_sof_zEstimate of the depth using MAG_SOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes]real
ebv_lenz17E(B-V) reddening coefficient map from Lenz et al. (2017)real
ebv_planck13E(B-V) reddening coefficient map from Planck Collaboration (2014)real
ebv_sfd98E(B-V) reddening coefficient map from Schlegel, Finkbeiner & Davis (1998)real
exptime_sum_gExposure time [s]real
exptime_sum_iExposure time [s]real
exptime_sum_rExposure time [s]real
exptime_sum_yExposure time [s]real
exptime_sum_zExposure time [s]real
fgcm_gry_min_gResidual "gray" corrections to the zeropoint from FGCM [mag] MINreal
fgcm_gry_min_iResidual "gray" corrections to the zeropoint from FGCM [mag] MINreal
fgcm_gry_min_rResidual "gray" corrections to the zeropoint from FGCM [mag] MINreal
fgcm_gry_min_yResidual "gray" corrections to the zeropoint from FGCM [mag] MINreal
fgcm_gry_min_zResidual "gray" corrections to the zeropoint from FGCM [mag] MINreal
fgcm_gry_wmean_gResidual "gray" corrections to the zeropoint from FGCM [mag] WMEANreal
fgcm_gry_wmean_iResidual "gray" corrections to the zeropoint from FGCM [mag] WMEANreal
fgcm_gry_wmean_rResidual "gray" corrections to the zeropoint from FGCM [mag] WMEANreal
fgcm_gry_wmean_yResidual "gray" corrections to the zeropoint from FGCM [mag] WMEANreal
fgcm_gry_wmean_zResidual "gray" corrections to the zeropoint from FGCM [mag] WMEANreal
fwhm_fluxrad_max_gTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_max_iTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_max_rTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_max_yTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_max_zTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_min_gTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_min_iTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_min_rTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_min_yTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_min_zTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_wmean_gTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_wmean_iTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_wmean_rTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_wmean_yTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_fluxrad_wmean_zTwice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec]real
fwhm_max_gAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_max_iAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_max_rAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_max_yAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_max_zAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_min_gAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_min_iAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_min_rAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_min_yAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_min_zAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_wmean_gAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_wmean_iAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_wmean_rAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_wmean_yAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
fwhm_wmean_zAverage FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec]real
hpix_4096Healpix ID for this entry, on NSIDE = 4096real
maglim_gMagnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag]real
maglim_iMagnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag]real
maglim_rMagnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag]real
maglim_yMagnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag]real
maglim_zMagnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag]real
n_images_gNumber of images.real
n_images_iNumber of images.real
n_images_rNumber of images.real
n_images_yNumber of images.real
n_images_zNumber of images.real
random_idRandom ID in the range 0.0 => 100.0real
sigma_mag_zero_qsum_gQuadrature sum of zeropoint uncertainties. [magnitudes]real
sigma_mag_zero_qsum_iQuadrature sum of zeropoint uncertainties. [magnitudes]real
sigma_mag_zero_qsum_rQuadrature sum of zeropoint uncertainties. [magnitudes]real
sigma_mag_zero_qsum_yQuadrature sum of zeropoint uncertainties. [magnitudes]real
sigma_mag_zero_qsum_zQuadrature sum of zeropoint uncertainties. [magnitudes]real
skyvar_max_gVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_max_iVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_max_rVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_max_yVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_max_zVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_min_gVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_min_iVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_min_rVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_min_yVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_min_zVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_sqrt_wmean_gSquare root of sky variance. [e-/CCD pixel]real
skyvar_sqrt_wmean_iSquare root of sky variance. [e-/CCD pixel]real
skyvar_sqrt_wmean_rSquare root of sky variance. [e-/CCD pixel]real
skyvar_sqrt_wmean_ySquare root of sky variance. [e-/CCD pixel]real
skyvar_sqrt_wmean_zSquare root of sky variance. [e-/CCD pixel]real
skyvar_uncertainty_gSky variance with flux scaled by zeropoint [e-/s/coadd pixel]real
skyvar_uncertainty_iSky variance with flux scaled by zeropoint [e-/s/coadd pixel]real
skyvar_uncertainty_rSky variance with flux scaled by zeropoint [e-/s/coadd pixel]real
skyvar_uncertainty_ySky variance with flux scaled by zeropoint [e-/s/coadd pixel]real
skyvar_uncertainty_zSky variance with flux scaled by zeropoint [e-/s/coadd pixel]real
skyvar_wmean_gVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_wmean_iVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_wmean_rVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_wmean_yVariance on the sky brightness. [(e-/CCD pixel)**2]real
skyvar_wmean_zVariance on the sky brightness. [(e-/CCD pixel)**2]real
t_eff_exptime_sum_gExposure time multiplied by T_EFF [s]real
t_eff_exptime_sum_iExposure time multiplied by T_EFF [s]real
t_eff_exptime_sum_rExposure time multiplied by T_EFF [s]real
t_eff_exptime_sum_yExposure time multiplied by T_EFF [s]real
t_eff_exptime_sum_zExposure time multiplied by T_EFF [s]real
t_eff_max_gFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_max_iFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_max_rFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_max_yFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_max_zFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_min_gFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_min_iFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_min_rFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_min_yFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_min_zFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_wmean_gFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_wmean_iFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_wmean_rFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_wmean_yFigure of merit for quality of observations [e-/s/coadd pixel]real
t_eff_wmean_zFigure of merit for quality of observations [e-/s/coadd pixel]real