Index: trunk/ippToPsps/config/tables.ST.vot =================================================================== --- trunk/ippToPsps/config/tables.ST.vot (revision 39067) +++ trunk/ippToPsps/config/tables.ST.vot (revision 39081) @@ -6,5 +6,9 @@ - Contains the metadata describing the stacked image produced from a set of single epoch exposures. The astrometric and photometric calibration of the stacked image are listed. + Contains the metadata describing the stacked image + produced from the combination of a set of single epoch + exposures. The nature of the stack is given by the StackTypeID. + The astrometric and photometric calibration of the stacked image + are listed. @@ -94,7 +98,4 @@ Locally derived photometric zero point for this stack. - - - Locally derived photometric color term for this stack. @@ -170,7 +171,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -207,4 +205,7 @@ Declination error from g filter stack detection. + + Modified Julian Date of the mean epoch of images contributing to the the g-band stack (equinox J2000). + PSF magnitude from g filter stack detection. @@ -260,4 +261,7 @@ Declination error from r filter stack detection. + + Modified Julian Date of the mean epoch of images contributing to the the r-band stack (equinox J2000). + PSF magnitude from r filter stack detection. @@ -313,4 +317,7 @@ Declination error from i filter stack detection. + + Modified Julian Date of the mean epoch of images contributing to the the i-band stack (equinox J2000). + PSF magnitude from i filter stack detection. @@ -366,4 +373,7 @@ Declination error from z filter stack detection. + + Modified Julian Date of the mean epoch of images contributing to the the z-band stack (equinox J2000). + PSF magnitude from z filter stack detection. @@ -418,4 +428,7 @@ Declination error from y filter stack detection. + + + Modified Julian Date of the mean epoch of images contributing to the the y-band stack (equinox J2000). @@ -470,7 +483,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -1021,5 +1031,5 @@
- Contains the unconvolved fluxes within the SDSS R5 (r = 3.00 arcsec), R6 (r = 4.63 arcsec), and R7 (r = 7.43 arcsec) apertures (Stoughton 2002). Convolved fluxes within these same apertures are also provided for convolution targets of 6 sky pixels (1.5 arcsec) and 8 sky pixels (2.0 arcsec). All filters are matched into a single row. See StackObjectThin table for discussion of primary, secondary, and best detections. References: Stoughton, C., Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 485. + Contains the unconvolved fluxes within the SDSS R5 (r = 3.00 arcsec), R6 (r = 4.63 arcsec), and R7 (r = 7.43 arcsec) apertures (Stoughton 2002). Convolved fluxes within these same apertures are also provided for images convolved to 6 sky pixels (1.5 arcsec) and 8 sky pixels (2.0 arcsec). All filters are matched into a single row. See StackObjectThin table for discussion of primary, secondary, and best detections. References: Stoughton, C., Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 485. @@ -1034,7 +1044,4 @@ Random value drawn from the interval between zero and one. - - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. @@ -1660,7 +1667,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -1845,7 +1849,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -2126,7 +2127,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -2407,7 +2405,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -2704,5 +2699,18 @@
- Contains the unconvolved fluxes within the SDSS R3 (r = 1.03 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 arcsec) apertures (Stoughton 2002) for extended sources. See StackObjectThin table for discussion of primary, secondary, and best detections. References: Stoughton, C., Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 485. + + Contains the unconvolved fluxes within the SDSS R3 + (r = 1.03 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), + R6 (r = 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 + arcsec), R9 (r = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 + (r = 44.21 arcsec) apertures (Stoughton 2002) for extended + sources. These measurements are only provided for objects in + the extragalactic sky, i.e., they are not provided for objects + in the Galactic plane because they are not useful in crowded + areas. See StackObjectThin table for discussion of primary, + secondary, and best detections. References: Stoughton, C., + Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, + 485. + @@ -2717,7 +2725,4 @@ Random value drawn from the interval between zero and one. - - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. @@ -3329,5 +3334,19 @@
- Contains the fluxes within the SDSS R3 (r = 1.03 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 arcsec) apertures (Stoughton 2002) for extended sources after the images have been convolved to a target of 6 sky pixels (1.5 arcsec). See StackObjectThin table for discussion of primary, secondary, and best detections. References: Stoughton, C., Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 485. + + Contains the fluxes within the SDSS R3 (r = 1.03 + arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = + 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r + = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 + arcsec) apertures (Stoughton 2002) for extended sources after + the images have been convolved to a target of 6 sky pixels (1.5 + arcsec). These measurements are only provided for objects in + the extragalactic sky, i.e., they are not provided for objects + in the Galactic plane because they are not useful in crowded + areas. See StackObjectThin table for discussion of primary, + secondary, and best detections. References: Stoughton, C., + Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, + 485. + @@ -3342,7 +3361,4 @@ Random value drawn from the interval between zero and one. - - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. @@ -3955,5 +3971,19 @@
- Contains the fluxes within the SDSS R3 (r = 1.03 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 arcsec) apertures (Stoughton 2002) for extended sources after the images have been convolved to a target of 8 sky pixels (2.0 arcsec). See StackObjectThin table for discussion of primary, secondary, and best detections. References: Stoughton, C., Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 485. + + Contains the fluxes within the SDSS R3 (r = 1.03 + arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = + 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r + = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 + arcsec) apertures (Stoughton 2002) for extended sources after + the images have been convolved to a target of 8 sky pixels (2.0 + arcsec). These measurements are only provided for objects in + the extragalactic sky, i.e., they are not provided for objects + in the Galactic plane because they are not useful in crowded + areas. See StackObjectThin table for discussion of primary, + secondary, and best detections. References: Stoughton, C., + Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, + 485. + @@ -3968,7 +3998,4 @@ Random value drawn from the interval between zero and one. - - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. @@ -4595,7 +4622,4 @@ Random value drawn from the interval between zero and one. - - Identifies if this row is the primary detection, a secondary detection, and if it is the best detection. - Identifies if this row is the primary stack detection. @@ -4844,5 +4868,10 @@
- Contains the detection efficiency information for a given stacked image. Provides the number of recovered sources out of 500 and statistics about the magnitudes of the recovered sources for a range of magnitude offsets. + + Contains the detection efficiency information for a + given stacked image. Provides the number of recovered sources + out of 500 injected sources for each magnitude bin and statistics about the magnitudes of the recovered + sources for a range of magnitude offsets. + @@ -4851,4 +4880,7 @@ Detection efficiency reference magnitude. + + + Number of fake sources injected in each magnitude bin.