Index: trunk/ippToPsps/config/tables.DF.vot =================================================================== --- trunk/ippToPsps/config/tables.DF.vot (revision 39087) +++ trunk/ippToPsps/config/tables.DF.vot (revision 39088) @@ -5,10 +5,5 @@ - Contains metadata related to a difference image - constructed by subtracting a stacked image from a single epoch - image, or in the case of the MD Survey from a nightly stack - (stack made from all exposures in a single filter in a single - night). The astrometric calibration of the reference stack is - listed. + Contains metadata related to a difference image constructed by subtracting a stacked image from a single epoch image, or in the case of the MD Survey from a nightly stack (stack made from all exposures in a single filter in a single night). The astrometric calibration of the reference stack is listed. @@ -32,5 +27,5 @@ - Image identifier for the positive image. For warp-stack difference images, this corresponds to the ForcedWarpToImage.forcedWarpID entry. For stack-stack difference images, this corresponds to StackMeta.stackImageID. + Image identifier for the positive image. For warp-stack difference images, this corresponds to the ForcedWarpToImage.forcedWarpID entry. For stack-stack difference images, this corresponds to StackMeta.stackImageID. Index: trunk/ippToPsps/config/tables.FO.vot =================================================================== --- trunk/ippToPsps/config/tables.FO.vot (revision 39087) +++ trunk/ippToPsps/config/tables.FO.vot (revision 39088) @@ -4,16 +4,5 @@
- Contains the mean of single-epoch photometric - information for sources detected in the stacked data, calculated - as described in Magnier et al. (2013). The mean is calculated - for detections associated into objects within a one arcsecond - correlation radius. PSF, Kron (1980), and SDSS aperture R5 (r = - 3.00 arcsec), R6 (r = 4.63 arcsec), and R7 (r = 7.43 arcsec) - apertures (Stoughton 2002) magnitudes and statistics are listed - for all filters. References: Kaiser, N., Squires, G., and - Broadhurst, T. 1995, ApJ, 449, 460; Kron, R. G. 1980, ApJS, 43, - 305; Magnier, E. A., Schlafly, E., Finkbeiner, D., et al. 2013, - ApJS, 205, 20; Stoughton, C., Lupton, R. H., Bernardi, M., et - al. 2002, AJ, 123, 485.. + Contains the mean of single-epoch photometric information for sources detected in the stacked data, calculated as described in Magnier et al. (2013). The mean is calculated for detections associated into objects within a one arcsecond correlation radius. PSF, Kron (1980), and SDSS aperture R5 (r = 3.00 arcsec), R6 (r = 4.63 arcsec), and R7 (r = 7.43 arcsec) apertures (Stoughton 2002) magnitudes and statistics are listed for all filters. References: Kaiser, N., Squires, G., and Broadhurst, T. 1995, ApJ, 449, 460; Kron, R. G. 1980, ApJS, 43, 305; Magnier, E. A., Schlafly, E., Finkbeiner, D., et al. 2013, ApJS, 205, 20; Stoughton, C., Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 485. Index: trunk/ippToPsps/config/tables.FW.vot =================================================================== --- trunk/ippToPsps/config/tables.FW.vot (revision 39087) +++ trunk/ippToPsps/config/tables.FW.vot (revision 39088) @@ -126,11 +126,5 @@
- Contains single epoch forced photometry of - individual measurements of objects detected in the stacked - images. The identifiers connecting the measurement back to the - original image and to the object association are provided. PSF, - aperture, and Kron (1980) photometry are included, along with - sky and detector coordinate positions. References: Kron, - R. G. 1980, ApJS, 43, 305. + Contains single epoch forced photometry of individual measurements of objects detected in the stacked images. The identifiers connecting the measurement back to the original image and to the object association are provided. PSF, aperture, and Kron (1980) photometry are included, along with sky and detector coordinate positions. References: Kron, R. G. 1980, ApJS, 43, 305. Index: trunk/ippToPsps/config/tables.IN.vot =================================================================== --- trunk/ippToPsps/config/tables.IN.vot (revision 39087) +++ trunk/ippToPsps/config/tables.IN.vot (revision 39088) @@ -23,10 +23,5 @@
- - Contains descriptions of the models used in fitting detections - in images, both PSF-like and extended galaxies. References: - de Vaucouleurs, G. 1948, Annales d'Astrophysique, 11, 247; - Sersic, J. L. 1963, Boletin de la Asociacion Argentina de - Astronomia La Plata Argentina, 6, 41. + Contains descriptions of the models used in fitting detections in images, both PSF-like and extended galaxies. References: de Vaucouleurs, G. 1948, Annales d'Astrophysique, 11, 247; Sersic, J. L. 1963, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 6, 41. Index: trunk/ippToPsps/config/tables.OB.vot =================================================================== --- trunk/ippToPsps/config/tables.OB.vot (revision 39087) +++ trunk/ippToPsps/config/tables.OB.vot (revision 39088) @@ -5,15 +5,5 @@
- Contains the positional information for objects in - a number of coordinate systems. The objects associate single - epoch detections and the stacked detections within a one - arcsecond radius. The mean position from the single epoch data - is used as the basis for coordinates when available, or the - position of an object in the stack when it is not. The right - ascension and declination for both the stack and single epoch - mean is provided. The number of detections in each filter from - single epoch data is listed, along with which filters the object - has a stack detection. References: Szalay, A. S., Gray, J., - Fekete, G., et al. 2007, arXiv:cs/0701164. + Contains the positional information for objects in a number of coordinate systems. The objects associate single epoch detections and the stacked detections within a one arcsecond radius. The mean position from the single epoch data is used as the basis for coordinates when available, or the position of an object in the stack when it is not. The right ascension and declination for both the stack and single epoch mean is provided. The number of detections in each filter from single epoch data is listed, along with which filters the object has a stack detection. References: Szalay, A. S., Gray, J., Fekete, G., et al. 2007, arXiv:cs/0701164. @@ -156,13 +146,5 @@
- Contains the mean photometric information for - objects based on the single epoch data, calculated as described - in Magnier et al (2013). To be included in this table, an - object must be bright enough to have been detected at least once - in an individual exposure. PSF, Kron (1980), and aperture - magnitudes and statistics are listed for all filters. - References: Kron, R. G. 1980, ApJS, 43, 305; Magnier, E. A., - Schlafly, E., Finkbeiner, D., et al. 2013, ApJS, 205, - 20. + Contains the mean photometric information for objects based on the single epoch data, calculated as described in Magnier et al (2013). To be included in this table, an object must be bright enough to have been detected at least once in an individual exposure. PSF, Kron (1980), and aperture magnitudes and statistics are listed for all filters. References: Kron, R. G. 1980, ApJS, 43, 305; Magnier, E. A., Schlafly, E., Finkbeiner, D., et al. 2013, ApJS, 205, 20. Index: trunk/ippToPsps/config/tables.P2.vot =================================================================== --- trunk/ippToPsps/config/tables.P2.vot (revision 39087) +++ trunk/ippToPsps/config/tables.P2.vot (revision 39088) @@ -4,10 +4,5 @@
- Contains metadata related to an individual - exposure. A "Frame" refers to the collection of all images - obtained by the 60 OTA devices in the camera in a single - exposure. The camera configuration, telescope pointing, - observation time, and astrometric solution from the detector - focal plane (L,M) to the sky (RA,Dec) is provided. + Contains metadata related to an individual exposure. A "Frame" refers to the collection of all images obtained by the 60 OTA devices in the camera in a single exposure. The camera configuration, telescope pointing, observation time, and astrometric solution from the detector focal plane (L,M) to the sky (RA,Dec) is provided. Index: trunk/ippToPsps/config/tables.ST.vot =================================================================== --- trunk/ippToPsps/config/tables.ST.vot (revision 39087) +++ 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.