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Table: des_dr1.y3_gold_surveyconditions
(The bold columns are indexed columns)
| Column Name | Description | Datatype |
|---|---|---|
| airmass_max_g | Secant of the max zenith angle | REAL |
| airmass_max_i | Secant of the max zenith angle | REAL |
| airmass_max_r | Secant of the max zenith angle | REAL |
| airmass_max_y | Secant of the max zenith angle | REAL |
| airmass_max_z | Secant of the max zenith angle | REAL |
| airmass_min_g | Secant of the min zenith angle | REAL |
| airmass_min_i | Secant of the min zenith angle | REAL |
| airmass_min_r | Secant of the min zenith angle | REAL |
| airmass_min_y | Secant of the min zenith angle | REAL |
| airmass_min_z | Secant of the min zenith angle | REAL |
| airmass_wmean_g | Secant of the mean zenith angle | REAL |
| airmass_wmean_i | Secant of the mean zenith angle | REAL |
| airmass_wmean_r | Secant of the mean zenith angle | REAL |
| airmass_wmean_y | Secant of the mean zenith angle | REAL |
| airmass_wmean_z | Secant of the mean zenith angle | REAL |
| depth_auto_g | Estimate 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_i | Estimate 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_r | Estimate 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_y | Estimate 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_z | Estimate 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_g | Estimate 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_i | Estimate 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_r | Estimate 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_z | Estimate 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_g | Estimate 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_i | Estimate 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_r | Estimate 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_z | Estimate of the depth using MAG_SOF photometry using a trained model. See section 5.1 of Sevilla-Noarbe et al. (2021) [magnitudes] | REAL |
| ebv_lenz17 | E(B-V) reddening coefficient map from Lenz et al. (2017) | REAL |
| ebv_planck13 | E(B-V) reddening coefficient map from Planck Collaboration (2014) | REAL |
| ebv_sfd98 | E(B-V) reddening coefficient map from Schlegel, Finkbeiner & Davis (1998) | REAL |
| exptime_sum_g | Exposure time [s] | REAL |
| exptime_sum_i | Exposure time [s] | REAL |
| exptime_sum_r | Exposure time [s] | REAL |
| exptime_sum_y | Exposure time [s] | REAL |
| exptime_sum_z | Exposure time [s] | REAL |
| fgcm_gry_min_g | Residual "gray" corrections to the zeropoint from FGCM [mag] MIN | REAL |
| fgcm_gry_min_i | Residual "gray" corrections to the zeropoint from FGCM [mag] MIN | REAL |
| fgcm_gry_min_r | Residual "gray" corrections to the zeropoint from FGCM [mag] MIN | REAL |
| fgcm_gry_min_y | Residual "gray" corrections to the zeropoint from FGCM [mag] MIN | REAL |
| fgcm_gry_min_z | Residual "gray" corrections to the zeropoint from FGCM [mag] MIN | REAL |
| fgcm_gry_wmean_g | Residual "gray" corrections to the zeropoint from FGCM [mag] WMEAN | REAL |
| fgcm_gry_wmean_i | Residual "gray" corrections to the zeropoint from FGCM [mag] WMEAN | REAL |
| fgcm_gry_wmean_r | Residual "gray" corrections to the zeropoint from FGCM [mag] WMEAN | REAL |
| fgcm_gry_wmean_y | Residual "gray" corrections to the zeropoint from FGCM [mag] WMEAN | REAL |
| fgcm_gry_wmean_z | Residual "gray" corrections to the zeropoint from FGCM [mag] WMEAN | REAL |
| fwhm_fluxrad_max_g | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_max_i | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_max_r | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_max_y | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_max_z | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_min_g | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_min_i | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_min_r | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_min_y | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_min_z | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_wmean_g | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_wmean_i | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_wmean_r | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_wmean_y | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_fluxrad_wmean_z | Twice the average half-light radius from the sources used for determining the PSF with PSFEx. [arcsec] | REAL |
| fwhm_max_g | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_max_i | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_max_r | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_max_y | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_max_z | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_min_g | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_min_i | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_min_r | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_min_y | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_min_z | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_wmean_g | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_wmean_i | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_wmean_r | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_wmean_y | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| fwhm_wmean_z | Average FWHM of the 2D elliptical Moffat function that fits best the PSF model from PSFEx. [arcsec] | REAL |
| hpix_4096 | Healpix ID for this entry, on NSIDE = 4096 | REAL |
| maglim_g | Magnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag] | REAL |
| maglim_i | Magnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag] | REAL |
| maglim_r | Magnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag] | REAL |
| maglim_y | Magnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag] | REAL |
| maglim_z | Magnitude limit estimated by mangle from the weight maps. This is measured as 10-sigma values in 2 arcsec diameter apertures. [mag] | REAL |
| n_images_g | Number of images. | REAL |
| n_images_i | Number of images. | REAL |
| n_images_r | Number of images. | REAL |
| n_images_y | Number of images. | REAL |
| n_images_z | Number of images. | REAL |
| random_id | Random ID in the range 0.0 => 100.0 | REAL |
| sigma_mag_zero_qsum_g | Quadrature sum of zeropoint uncertainties. [magnitudes] | REAL |
| sigma_mag_zero_qsum_i | Quadrature sum of zeropoint uncertainties. [magnitudes] | REAL |
| sigma_mag_zero_qsum_r | Quadrature sum of zeropoint uncertainties. [magnitudes] | REAL |
| sigma_mag_zero_qsum_y | Quadrature sum of zeropoint uncertainties. [magnitudes] | REAL |
| sigma_mag_zero_qsum_z | Quadrature sum of zeropoint uncertainties. [magnitudes] | REAL |
| skyvar_max_g | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_max_i | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_max_r | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_max_y | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_max_z | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_min_g | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_min_i | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_min_r | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_min_y | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_min_z | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_sqrt_wmean_g | Square root of sky variance. [e-/CCD pixel] | REAL |
| skyvar_sqrt_wmean_i | Square root of sky variance. [e-/CCD pixel] | REAL |
| skyvar_sqrt_wmean_r | Square root of sky variance. [e-/CCD pixel] | REAL |
| skyvar_sqrt_wmean_y | Square root of sky variance. [e-/CCD pixel] | REAL |
| skyvar_sqrt_wmean_z | Square root of sky variance. [e-/CCD pixel] | REAL |
| skyvar_uncertainty_g | Sky variance with flux scaled by zeropoint [e-/s/coadd pixel] | REAL |
| skyvar_uncertainty_i | Sky variance with flux scaled by zeropoint [e-/s/coadd pixel] | REAL |
| skyvar_uncertainty_r | Sky variance with flux scaled by zeropoint [e-/s/coadd pixel] | REAL |
| skyvar_uncertainty_y | Sky variance with flux scaled by zeropoint [e-/s/coadd pixel] | REAL |
| skyvar_uncertainty_z | Sky variance with flux scaled by zeropoint [e-/s/coadd pixel] | REAL |
| skyvar_wmean_g | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_wmean_i | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_wmean_r | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_wmean_y | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| skyvar_wmean_z | Variance on the sky brightness. [(e-/CCD pixel)**2] | REAL |
| t_eff_exptime_sum_g | Exposure time multiplied by T_EFF [s] | REAL |
| t_eff_exptime_sum_i | Exposure time multiplied by T_EFF [s] | REAL |
| t_eff_exptime_sum_r | Exposure time multiplied by T_EFF [s] | REAL |
| t_eff_exptime_sum_y | Exposure time multiplied by T_EFF [s] | REAL |
| t_eff_exptime_sum_z | Exposure time multiplied by T_EFF [s] | REAL |
| t_eff_max_g | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_max_i | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_max_r | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_max_y | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_max_z | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_min_g | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_min_i | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_min_r | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_min_y | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_min_z | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_wmean_g | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_wmean_i | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_wmean_r | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_wmean_y | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
| t_eff_wmean_z | Figure of merit for quality of observations [e-/s/coadd pixel] | REAL |
