Index: trunk/ippToPsps/config/tables.ST.vot =================================================================== --- trunk/ippToPsps/config/tables.ST.vot (revision 39081) +++ trunk/ippToPsps/config/tables.ST.vot (revision 39088) @@ -6,9 +6,5 @@ - 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. + 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. @@ -2700,16 +2696,5 @@
- 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. + 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. @@ -3335,17 +3320,5 @@
- 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. + 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. @@ -3972,17 +3945,5 @@
- 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. + 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. @@ -4869,8 +4830,5 @@
- 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. + 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.