Changeset 39081 for trunk/ippToPsps/config/tables.ST.vot
- Timestamp:
- Nov 9, 2015, 11:48:04 AM (11 years ago)
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- 1 edited
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trunk/ippToPsps/config/tables.ST.vot (modified) (24 diffs)
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trunk/ippToPsps/config/tables.ST.vot
r39067 r39081 6 6 <!-- StackMeta Table ************************************************** --> 7 7 <TABLE name="StackMeta"> 8 <DESCRIPTION>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.</DESCRIPTION> 8 <DESCRIPTION>Contains the metadata describing the stacked image 9 produced from the combination of a set of single epoch 10 exposures. The nature of the stack is given by the StackTypeID. 11 The astrometric and photometric calibration of the stacked image 12 are listed.</DESCRIPTION> 9 13 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 10 14 <FIELD name="stackImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 94 98 <FIELD name="photoZero" arraysize="1" datatype="float" unit="magnitudes" default="-999"> 95 99 <DESCRIPTION>Locally derived photometric zero point for this stack.</DESCRIPTION> 96 </FIELD>97 <FIELD name="photoColor" arraysize="1" datatype="float" unit="magnitudes" default="-999">98 <DESCRIPTION>Locally derived photometric color term for this stack.</DESCRIPTION>99 100 </FIELD> 100 101 <FIELD name="ctype1" arraysize="100" datatype="char" unit="dimensionless" default=""> … … 170 171 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 171 172 </FIELD> 172 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">173 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>174 </FIELD>175 173 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 176 174 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 207 205 <DESCRIPTION>Declination error from g filter stack detection.</DESCRIPTION> 208 206 </FIELD> 207 <FIELD name="gEpoch" arraysize="1" datatype="double" unit="days" default="-999"> 208 <DESCRIPTION>Modified Julian Date of the mean epoch of images contributing to the the g-band stack (equinox J2000).</DESCRIPTION> 209 </FIELD> 209 210 <FIELD name="gPSFMag" arraysize="1" datatype="float" unit="AB magnitudes" default="-999"> 210 211 <DESCRIPTION>PSF magnitude from g filter stack detection.</DESCRIPTION> … … 260 261 <DESCRIPTION>Declination error from r filter stack detection.</DESCRIPTION> 261 262 </FIELD> 263 <FIELD name="rEpoch" arraysize="1" datatype="double" unit="days" default="-999"> 264 <DESCRIPTION>Modified Julian Date of the mean epoch of images contributing to the the r-band stack (equinox J2000).</DESCRIPTION> 265 </FIELD> 262 266 <FIELD name="rPSFMag" arraysize="1" datatype="float" unit="AB magnitudes" default="-999"> 263 267 <DESCRIPTION>PSF magnitude from r filter stack detection.</DESCRIPTION> … … 313 317 <DESCRIPTION>Declination error from i filter stack detection.</DESCRIPTION> 314 318 </FIELD> 319 <FIELD name="iEpoch" arraysize="1" datatype="double" unit="days" default="-999"> 320 <DESCRIPTION>Modified Julian Date of the mean epoch of images contributing to the the i-band stack (equinox J2000).</DESCRIPTION> 321 </FIELD> 315 322 <FIELD name="iPSFMag" arraysize="1" datatype="float" unit="AB magnitudes" default="-999"> 316 323 <DESCRIPTION>PSF magnitude from i filter stack detection.</DESCRIPTION> … … 366 373 <DESCRIPTION>Declination error from z filter stack detection.</DESCRIPTION> 367 374 </FIELD> 375 <FIELD name="zEpoch" arraysize="1" datatype="double" unit="days" default="-999"> 376 <DESCRIPTION>Modified Julian Date of the mean epoch of images contributing to the the z-band stack (equinox J2000).</DESCRIPTION> 377 </FIELD> 368 378 <FIELD name="zPSFMag" arraysize="1" datatype="float" unit="AB magnitudes" default="-999"> 369 379 <DESCRIPTION>PSF magnitude from z filter stack detection.</DESCRIPTION> … … 418 428 <FIELD name="ydecErr" arraysize="1" datatype="float" unit="arcsec" default="-999"> 419 429 <DESCRIPTION>Declination error from y filter stack detection.</DESCRIPTION> 430 </FIELD> 431 <FIELD name="yEpoch" arraysize="1" datatype="double" unit="days" default="-999"> 432 <DESCRIPTION>Modified Julian Date of the mean epoch of images contributing to the the y-band stack (equinox J2000).</DESCRIPTION> 420 433 </FIELD> 421 434 <FIELD name="yPSFMag" arraysize="1" datatype="float" unit="AB magnitudes" default="-999"> … … 470 483 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 471 484 </FIELD> 472 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">473 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>474 </FIELD>475 485 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 476 486 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 1021 1031 <!-- StackApFlx Table ************************************************** --> 1022 1032 <TABLE name="StackApFlx"> 1023 <DESCRIPTION>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 of6 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.</DESCRIPTION>1033 <DESCRIPTION>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.</DESCRIPTION> 1024 1034 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 1025 1035 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 1034 1044 <FIELD name="randomStackObjID" arraysize="1" datatype="double" unit="dimensionless" default="NA"> 1035 1045 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 1036 </FIELD>1037 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">1038 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>1039 1046 </FIELD> 1040 1047 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> … … 1660 1667 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 1661 1668 </FIELD> 1662 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">1663 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>1664 </FIELD>1665 1669 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 1666 1670 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 1845 1849 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 1846 1850 </FIELD> 1847 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">1848 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>1849 </FIELD>1850 1851 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 1851 1852 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 2126 2127 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 2127 2128 </FIELD> 2128 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">2129 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>2130 </FIELD>2131 2129 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 2132 2130 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 2407 2405 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 2408 2406 </FIELD> 2409 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">2410 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>2411 </FIELD>2412 2407 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 2413 2408 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 2704 2699 <!-- StackApFlxFull Table ************************************************** --> 2705 2700 <TABLE name="StackApFlxExGalUnc"> 2706 <DESCRIPTION>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.</DESCRIPTION> 2701 2702 <DESCRIPTION>Contains the unconvolved fluxes within the SDSS R3 2703 (r = 1.03 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), 2704 R6 (r = 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 2705 arcsec), R9 (r = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 2706 (r = 44.21 arcsec) apertures (Stoughton 2002) for extended 2707 sources. These measurements are only provided for objects in 2708 the extragalactic sky, i.e., they are not provided for objects 2709 in the Galactic plane because they are not useful in crowded 2710 areas. See StackObjectThin table for discussion of primary, 2711 secondary, and best detections. References: Stoughton, C., 2712 Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 2713 485.</DESCRIPTION> 2714 2707 2715 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 2708 2716 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 2717 2725 <FIELD name="randomStackObjID" arraysize="1" datatype="double" unit="dimensionless" default="NA"> 2718 2726 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 2719 </FIELD>2720 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">2721 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>2722 2727 </FIELD> 2723 2728 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> … … 3329 3334 <!-- StackApFlxFullC6 Table ************************************************** --> 3330 3335 <TABLE name="StackApFlxExGalCon6"> 3331 <DESCRIPTION>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.</DESCRIPTION> 3336 3337 <DESCRIPTION>Contains the fluxes within the SDSS R3 (r = 1.03 3338 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = 3339 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r 3340 = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 3341 arcsec) apertures (Stoughton 2002) for extended sources after 3342 the images have been convolved to a target of 6 sky pixels (1.5 3343 arcsec). These measurements are only provided for objects in 3344 the extragalactic sky, i.e., they are not provided for objects 3345 in the Galactic plane because they are not useful in crowded 3346 areas. See StackObjectThin table for discussion of primary, 3347 secondary, and best detections. References: Stoughton, C., 3348 Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 3349 485.</DESCRIPTION> 3350 3332 3351 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 3333 3352 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 3342 3361 <FIELD name="randomStackObjID" arraysize="1" datatype="double" unit="dimensionless" default="NA"> 3343 3362 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 3344 </FIELD>3345 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">3346 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>3347 3363 </FIELD> 3348 3364 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> … … 3955 3971 <!-- StackApFlxFullC8 Table ************************************************** --> 3956 3972 <TABLE name="StackApFlxExGalCon8"> 3957 <DESCRIPTION>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.</DESCRIPTION> 3973 3974 <DESCRIPTION>Contains the fluxes within the SDSS R3 (r = 1.03 3975 arcsec), R4 (r = 1.76 arcsec), R5 (r = 3.00 arcsec), R6 (r = 3976 4.63 arcsec), R7 (r = 7.43 arcsec), R8 (r = 11.42 arcsec), R9 (r 3977 = 18.20 arcsec), R10 (r = 28.20 arcsec), and R11 (r = 44.21 3978 arcsec) apertures (Stoughton 2002) for extended sources after 3979 the images have been convolved to a target of 8 sky pixels (2.0 3980 arcsec). These measurements are only provided for objects in 3981 the extragalactic sky, i.e., they are not provided for objects 3982 in the Galactic plane because they are not useful in crowded 3983 areas. See StackObjectThin table for discussion of primary, 3984 secondary, and best detections. References: Stoughton, C., 3985 Lupton, R. H., Bernardi, M., et al. 2002, AJ, 123, 3986 485.</DESCRIPTION> 3987 3958 3988 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 3959 3989 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 3968 3998 <FIELD name="randomStackObjID" arraysize="1" datatype="double" unit="dimensionless" default="NA"> 3969 3999 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 3970 </FIELD>3971 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">3972 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>3973 4000 </FIELD> 3974 4001 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> … … 4595 4622 <DESCRIPTION>Random value drawn from the interval between zero and one.</DESCRIPTION> 4596 4623 </FIELD> 4597 <FIELD name="stackDetectRowID" arraysize="1" datatype="long" unit="dimensionless" default="NA">4598 <DESCRIPTION>Identifies if this row is the primary detection, a secondary detection, and if it is the best detection.</DESCRIPTION>4599 </FIELD>4600 4624 <FIELD name="primaryDetection" arraysize="1" datatype="unsignedByte" unit="dimensionless" default="255"> 4601 4625 <DESCRIPTION>Identifies if this row is the primary stack detection.</DESCRIPTION> … … 4844 4868 <!-- StackDetEffMeta Table ************************************************** --> 4845 4869 <TABLE name="StackDetEffMeta"> 4846 <DESCRIPTION>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.</DESCRIPTION> 4870 4871 <DESCRIPTION>Contains the detection efficiency information for a 4872 given stacked image. Provides the number of recovered sources 4873 out of 500 injected sources for each magnitude bin and statistics about the magnitudes of the recovered 4874 sources for a range of magnitude offsets.</DESCRIPTION> 4875 4847 4876 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 4848 4877 <FIELD name="stackImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 4851 4880 <FIELD name="magref" arraysize="1" datatype="float" unit="magnitudes" default="NA"> 4852 4881 <DESCRIPTION>Detection efficiency reference magnitude.</DESCRIPTION> 4882 </FIELD> 4883 <FIELD name="nInjected" arraysize="1" datatype="int" unit="dimensionless" default="NA"> 4884 <DESCRIPTION>Number of fake sources injected in each magnitude bin.</DESCRIPTION> 4853 4885 </FIELD> 4854 4886 <FIELD name="offset01" arraysize="1" datatype="float" unit="magnitudes" default="NA">
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