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Table: phat_v2.star_v2
(The bold columns are indexed columns)
| Column Name | Description | Datatype |
|---|---|---|
| dec | J2000 Declination of the source in decimal degrees | DOUBLE |
| f110w_chi | Goodness of fit to the PSF, in filter f110w | REAL |
| f110w_crowd | crowding of the source (difference that subtracting neighbors has on the measured magnitude of the source), in filter f110w | REAL |
| f110w_err | error in magnitudes, in filter f110w | REAL |
| f110w_flag | DOLPHOT quality flag, in filter f110w | SMALLINT |
| f110w_gst | Does the source pass the GST criteria of Williams et al. (2014)? In filter f110w | SMALLINT |
| f110w_rate | CTE-adjusted, aperture corrected count rate for the source in filter f110w | REAL |
| f110w_raterr | Error in rate, in filter f110w | REAL |
| f110w_round | Roundness of the source, in filter f110w | REAL |
| f110w_sharp | Sharpness of the source, in filter f110w | REAL |
| f110w_snr | Signal-to-noise ratio of the measurement, in filter f110w | REAL |
| f110w_vega | VEGA magnitude for the source, in filter f110w | REAL |
| f160w_chi | Goodness of fit to the PSF, in filter f160w | REAL |
| f160w_crowd | crowding of the source (difference that subtracting neighbors has on the measured magnitude of the source), in filter f160w | REAL |
| f160w_err | error in magnitudes, in filter f160w | REAL |
| f160w_flag | DOLPHOT quality flag, in filter f160w | SMALLINT |
| f160w_gst | Does the source pass the GST criteria of Williams et al. (2014)? In filter f160w | SMALLINT |
| f160w_rate | CTE-adjusted, aperture corrected count rate for the source in filter f160w | REAL |
| f160w_raterr | Error in rate, in filter f160w | REAL |
| f160w_round | Roundness of the source, in filter f160w | REAL |
| f160w_sharp | Sharpness of the source, in filter f160w | REAL |
| f160w_snr | Signal-to-noise ratio of the measurement, in filter f160w | REAL |
| f160w_vega | VEGA magnitude for the source, in filter f160w | REAL |
| f275w_chi | Goodness of fit to the PSF, in filter f275w | REAL |
| f275w_crowd | crowding of the source (difference that subtracting neighbors has on the measured magnitude of the source), in filter f275w | REAL |
| f275w_err | error in magnitudes, in filter f275w | REAL |
| f275w_flag | DOLPHOT quality flag, in filter f275w | SMALLINT |
| f275w_gst | Does the source pass the GST criteria of Williams et al. (2014)? In filter f275w | SMALLINT |
| f275w_rate | CTE-adjusted, aperture corrected count rate for the source in filter f275w | REAL |
| f275w_raterr | Error in rate, in filter f275w | REAL |
| f275w_round | Roundness of the source, in filter f275w | REAL |
| f275w_sharp | Sharpness of the source, in filter f275w | REAL |
| f275w_snr | Signal-to-noise ratio of the measurement, in filter f275w | REAL |
| f275w_vega | VEGA magnitude for the source, in filter f275w | REAL |
| f336w_chi | Goodness of fit to PSF, in filter f336w | REAL |
| f336w_crowd | crowding of the source (difference that subtracting neighbors has on the measured magnitude of the source), in filter f336w | REAL |
| f336w_err | error in magnitudes, in filter f336w | REAL |
| f336w_flag | DOLPHOT quality flag, in filter f336w | SMALLINT |
| f336w_gst | Does the source pass the GST criteria of Williams et al. (2014)? In filter f336w | SMALLINT |
| f336w_rate | CTE-adjusted, aperture corrected count rate for the source f336w | REAL |
| f336w_raterr | Error in rate, in filter f336w | REAL |
| f336w_round | Roundness of the source, in filter f336w | REAL |
| f336w_sharp | Sharpness of the source, in filter f336w | REAL |
| f336w_snr | Signal-to-noise ratio of the measurement, in filter f336w | REAL |
| f336w_vega | VEGA magnitude for the source, in filter f336w | REAL |
| f475w_chi | Goodness of fit to the PSF, in filter f475w | REAL |
| f475w_crowd | crowding of the source (difference that subtracting neighbors has on the measured magnitude of the source), in filter f475w | REAL |
| f475w_err | error in magnitudes, in filter f475w | REAL |
| f475w_flag | DOLPHOT quality flag, in filter f475w | SMALLINT |
| f475w_gst | Does the source pass the GST criteria of Williams et al. (2014)? In filter f475w | SMALLINT |
| f475w_rate | CTE-adjusted, aperture corrected count rate for the source f475w | REAL |
| f475w_raterr | Error in rate, in filter f475w | REAL |
| f475w_round | Roundness of the source, in filter f475w | REAL |
| f475w_sharp | Sharpness of the source, in filter f475w | REAL |
| f475w_snr | Signal-to-noise ratio of the measurement, in filter f475w | REAL |
| f475w_vega | VEGA magnitude for the source, in filter f475w | REAL |
| f814w_chi | Goodness of fit to the PSF, in filter f814w | REAL |
| f814w_crowd | crowding of the source (difference that subtracting neighbors has on the measured magnitude of the source), in filter f814w | REAL |
| f814w_err | error in magnitudes, in filter f814w | REAL |
| f814w_flag | DOLPHOT quality flag, in filter f814w | SMALLINT |
| f814w_gst | Does the source pass the GST criteria of Williams et al. (2014)? In filter f814w | SMALLINT |
| f814w_rate | CTE-adjusted, aperture corrected count rate for the source in filter f814w | REAL |
| f814w_raterr | Error in rate, in filter f814w | REAL |
| f814w_round | Roundness of the source, in filter f814w | REAL |
| f814w_sharp | Sharpness of the source, in filter f814w | REAL |
| f814w_snr | Signal-to-noise ratio of the measurement, in filter f814w | REAL |
| f814w_vega | VEGA magnitude for the source, in filter f814w | REAL |
| field | Field number | BIGINT |
| inside_brick | Was the source inside the defined brick region | SMALLINT |
| inside_chipgap | Was the source on the ACS chipgap of that field | SMALLINT |
| inside_ir | Was the source inside the IR footprint | SMALLINT |
| inside_other_chipgap | Was the source on the ACS chipgap of another field | SMALLINT |
| ir_x | X pixel position on the IR detector | REAL |
| ir_y | Y pixel position on the IR detector | REAL |
| ra | J2000 Right Ascension of the source in decimal degrees | DOUBLE |
| x | X value of the pixel position on the reference drizzled image | REAL |
| y | Y value of the pixel position on the reference drizzled image | REAL |
