Changeset 39081
- Timestamp:
- Nov 9, 2015, 11:48:04 AM (11 years ago)
- Location:
- trunk/ippToPsps/config
- Files:
-
- 8 edited
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schema_browser.vot (modified) (1 diff)
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tables.DF.vot (modified) (5 diffs)
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tables.FO.vot (modified) (1 diff)
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tables.FW.vot (modified) (3 diffs)
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tables.IN.vot (modified) (6 diffs)
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tables.OB.vot (modified) (5 diffs)
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tables.P2.vot (modified) (6 diffs)
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tables.ST.vot (modified) (24 diffs)
Legend:
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trunk/ippToPsps/config/schema_browser.vot
r39069 r39081 149 149 <TABLE name="FitModel"> </TABLE> 150 150 <TABLE name="Survey"> </TABLE> 151 <TABLE name="CameraConfig"> </TABLE>152 151 <TABLE name="PhotoCal"> </TABLE> 153 152 <TABLE name="StackType"> </TABLE> -
trunk/ippToPsps/config/tables.DF.vot
r39071 r39081 4 4 <RESOURCE> 5 5 <TABLE name="DiffMeta"> 6 <DESCRIPTION>Contains metadata related to a difference image constructed by subtracting the stacked image from the single epoch data. The astrometric calibration of the reference stack is listed.</DESCRIPTION> 6 7 <DESCRIPTION>Contains metadata related to a difference image 8 constructed by subtracting a stacked image from a single epoch 9 image, or in the case of the MD Survey from a nightly stack 10 (stack made from all exposures in a single filter in a single 11 night). The astrometric calibration of the reference stack is 12 listed.</DESCRIPTION> 13 7 14 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 8 15 <FIELD name="diffImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 22 29 </FIELD> 23 30 <FIELD name="frameID" arraysize="1" datatype="int" unit="dimensionless" default="NA"> 24 <DESCRIPTION>Frame/exposure identifier for the postitive image in warp-stack difference images .</DESCRIPTION>31 <DESCRIPTION>Frame/exposure identifier for the postitive image in warp-stack difference images; not populated for stack-stack differences.</DESCRIPTION> 25 32 </FIELD> 26 33 <FIELD name="posImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> 27 <DESCRIPTION>Image identifier for the positive image. For warp-stack difference images, this corresponds to the ForcedWarpToImage.forcedWarpID entry. </DESCRIPTION>34 <DESCRIPTION>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. </DESCRIPTION> 28 35 </FIELD> 29 36 <FIELD name="negImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 134 141 </TABLE> 135 142 <TABLE name="DiffDetection"> 136 <DESCRIPTION>Contains the photometry of individual detections from thedifference image. The identifiers connecting the detection back to the difference image and to the object association are provided. PSF, aperture, and Kron (1980) photometry are included, along with sky and detector coordinate positions. Statistics References: Kron, R. G. 1980, ApJS, 43, 305.</DESCRIPTION>143 <DESCRIPTION>Contains the photometry of individual detections from a difference image. The identifiers connecting the detection back to the difference image and to the object association are provided. PSF, aperture, and Kron (1980) photometry are included, along with sky and detector coordinate positions. Statistics References: Kron, R. G. 1980, ApJS, 43, 305.</DESCRIPTION> 137 144 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 138 145 <FIELD name="diffObjID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 356 363 357 364 <TABLE name="DiffDetEffMeta"> 358 <DESCRIPTION>Contains the detection efficiency information for a given individual difference 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>365 <DESCRIPTION>Contains the detection efficiency information for a given individual difference image. Provides the number of recovered sources out of 500 injected sources and statistics about the magnitudes of the recovered sources for a range of magnitude offsets.</DESCRIPTION> 359 366 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 360 367 <FIELD name="diffImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 363 370 <FIELD name="magref" arraysize="1" datatype="float" unit="magnitudes" default="NA"> 364 371 <DESCRIPTION>Detection efficiency reference magnitude.</DESCRIPTION> 372 </FIELD> 373 <FIELD name="nInjected" arraysize="1" datatype="int" unit="dimensionless" default="NA"> 374 <DESCRIPTION>Number of fake sources injected in each magnitude bin.</DESCRIPTION> 365 375 </FIELD> 366 376 <FIELD name="offset01" arraysize="1" datatype="float" unit="magnitudes" default="NA"> -
trunk/ippToPsps/config/tables.FO.vot
r38868 r39081 4 4 <RESOURCE> 5 5 <TABLE name="ForcedMeanObject"> 6 <DESCRIPTION>Contains the mean of single-epoch photometric information for object sources detected in the stacked data, calculated as described in Magnier et al. (2013). The objects associate forced warp detections within a one arcsecond 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..</DESCRIPTION> 6 <DESCRIPTION>Contains the mean of single-epoch photometric 7 information for sources detected in the stacked data, calculated 8 as described in Magnier et al. (2013). The mean is calculated 9 for detections associated into objects within a one arcsecond 10 correlation radius. PSF, Kron (1980), and SDSS aperture R5 (r = 11 3.00 arcsec), R6 (r = 4.63 arcsec), and R7 (r = 7.43 arcsec) 12 apertures (Stoughton 2002) magnitudes and statistics are listed 13 for all filters. References: Kaiser, N., Squires, G., and 14 Broadhurst, T. 1995, ApJ, 449, 460; Kron, R. G. 1980, ApJS, 43, 15 305; Magnier, E. A., Schlafly, E., Finkbeiner, D., et al. 2013, 16 ApJS, 205, 20; Stoughton, C., Lupton, R. H., Bernardi, M., et 17 al. 2002, AJ, 123, 485..</DESCRIPTION> 7 18 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 8 19 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> -
trunk/ippToPsps/config/tables.FW.vot
r38961 r39081 81 81 <DESCRIPTION>Locally derived photometric zero point for this warp image.</DESCRIPTION> 82 82 </FIELD> 83 <FIELD name="photoColor" arraysize="1" datatype="float" unit="magnitudes" default="-999">84 <DESCRIPTION>Locally derived photometric color term for this warp image.</DESCRIPTION>85 </FIELD>86 83 <FIELD name="ctype1" arraysize="100" datatype="char" unit="dimensionless" default=""> 87 84 <DESCRIPTION>Name of astrometric projection in right ascension.</DESCRIPTION> … … 128 125 </TABLE> 129 126 <TABLE name="ForcedWarpMeasurement"> 130 <DESCRIPTION>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. </DESCRIPTION> 127 128 <DESCRIPTION>Contains single epoch forced photometry of 129 individual measurements of objects detected in the stacked 130 images. The identifiers connecting the measurement back to the 131 original image and to the object association are provided. PSF, 132 aperture, and Kron (1980) photometry are included, along with 133 sky and detector coordinate positions. References: Kron, 134 R. G. 1980, ApJS, 43, 305. </DESCRIPTION> 135 131 136 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 132 137 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 294 299 </TABLE> 295 300 <TABLE name="ForcedWarpMasked"> 296 <DESCRIPTION>Contains single epoch forced photometry of objects detected in the stacked images but are masked in a particular warp image.</DESCRIPTION>301 <DESCRIPTION>Contains an entry for objects detected in the stacked images which were in the footprint of a single epoch exposure, but for which there are no unmasked pixels at that epoch.</DESCRIPTION> 297 302 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 298 303 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> -
trunk/ippToPsps/config/tables.IN.vot
r39066 r39081 4 4 <RESOURCE> 5 5 <TABLE name="Filter"> 6 <DESCRIPTION>Contains a description of the optical filters used in exposures.</DESCRIPTION>6 <DESCRIPTION>Contains a description of the optical filters used in the survey (Tonry et al 2012, ApJ 750, 99).</DESCRIPTION> 7 7 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 8 8 <FIELD name="filterID" arraysize="1" datatype="unsignedByte"> … … 11 11 <FIELD name="filterType" arraysize="100" datatype="char"> 12 12 <DESCRIPTION>Filter name.</DESCRIPTION> 13 </FIELD>14 <FIELD name="filterSpec" arraysize="100" datatype="char">15 <DESCRIPTION>Filter specifications.</DESCRIPTION>16 13 </FIELD> 17 14 <DATA> … … 26 23 </TABLE> 27 24 <TABLE name="FitModel"> 28 <DESCRIPTION>Contains descriptions of the models used in fitting detections. 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.</DESCRIPTION> 25 <DESCRIPTION> 26 Contains descriptions of the models used in fitting detections 27 in images, both PSF-like and extended galaxies. References: 28 de Vaucouleurs, G. 1948, Annales d'Astrophysique, 11, 247; 29 Sersic, J. L. 1963, Boletin de la Asociacion Argentina de 30 Astronomia La Plata Argentina, 6, 41.</DESCRIPTION> 29 31 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 30 32 <FIELD name="fitModelID" arraysize="1" datatype="short"> … … 82 84 </TABLE> 83 85 <TABLE name="Survey"> 84 <DESCRIPTION>Contains descriptions of the various project surveys.</DESCRIPTION>86 <DESCRIPTION>Contains descriptions of the various PS1 Science Consortium Surveys.</DESCRIPTION> 85 87 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 86 88 <FIELD name="surveyID" arraysize="1" datatype="unsignedByte"> … … 130 132 </DATA> 131 133 </TABLE> 132 <TABLE name="CameraConfig">133 <DESCRIPTION>Contains descriptions of the camera configuration changes.</DESCRIPTION>134 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>135 <FIELD name="cameraID" arraysize="1" datatype="short">136 <DESCRIPTION>Camera identifier.</DESCRIPTION>137 </FIELD>138 <FIELD name="cameraConfigID" arraysize="1" datatype="short">139 <DESCRIPTION>Camera configuration identifier.</DESCRIPTION>140 </FIELD>141 <FIELD name="endDate" arraysize="1" datatype="float" unit="days">142 <DESCRIPTION>Modified Julian Date of the end of this configuration.</DESCRIPTION>143 </FIELD>144 <FIELD name="configDetails" arraysize="100" datatype="char">145 <DESCRIPTION>Description of the camera configuration.</DESCRIPTION>146 </FIELD>147 <DATA>148 <TABLEDATA>149 <TR><TD>1</TD><TD>1</TD><TD>54000.0</TD></TR>150 <TR><TD>1</TD><TD>2</TD><TD>54000.0</TD><TD>f0123456789abcde</TD></TR>151 </TABLEDATA>152 </DATA>153 </TABLE>154 134 <TABLE name="PhotoCal"> 155 135 <DESCRIPTION>Contains photometric calibration information for each filter and detector image combinations.</DESCRIPTION> … … 164 144 <DESCRIPTION>Photometry reduction code name.</DESCRIPTION> 165 145 </FIELD> 166 <FIELD name="AB" arraysize="1" datatype="float" >146 <FIELD name="AB" arraysize="1" datatype="float" unit="magnitudes"> 167 147 <DESCRIPTION>AB magnitude.</DESCRIPTION> 168 148 </FIELD> 169 <FIELD name="zeropoint" arraysize="1" datatype="float" >149 <FIELD name="zeropoint" arraysize="1" datatype="float" unit="magnitudes"> 170 150 <DESCRIPTION>Photometric zeropoint (excluding long term variation).</DESCRIPTION> 171 151 </FIELD> 172 <FIELD name="extinction" arraysize="1" datatype="float" >152 <FIELD name="extinction" arraysize="1" datatype="float" unit="magnitudes / airmass"> 173 153 <DESCRIPTION>Photometric extinction term (excluding long term variation).</DESCRIPTION> 174 154 </FIELD> -
trunk/ippToPsps/config/tables.OB.vot
r39032 r39081 4 4 <RESOURCE> 5 5 <TABLE name="ObjectThin"> 6 <DESCRIPTION>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 position of an object in the stack is used as the basis for coordinates when available, with the mean position from the single epoch data 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.</DESCRIPTION> 6 7 <DESCRIPTION>Contains the positional information for objects in 8 a number of coordinate systems. The objects associate single 9 epoch detections and the stacked detections within a one 10 arcsecond radius. The mean position from the single epoch data 11 is used as the basis for coordinates when available, or the 12 position of an object in the stack when it is not. The right 13 ascension and declination for both the stack and single epoch 14 mean is provided. The number of detections in each filter from 15 single epoch data is listed, along with which filters the object 16 has a stack detection. References: Szalay, A. S., Gray, J., 17 Fekete, G., et al. 2007, arXiv:cs/0701164.</DESCRIPTION> 18 7 19 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 8 20 <FIELD name="objName" arraysize="32" datatype="char" unit="dimensionless" default="NA"> … … 64 76 </FIELD> 65 77 <FIELD name="raStack" arraysize="1" datatype="double" unit="degrees" default="-999"> 66 <DESCRIPTION>Right ascension mean from stack detections.</DESCRIPTION>78 <DESCRIPTION>Right ascension from stack detections, weighted mean value across filters, in equinox J2000. See StackObjectThin for stack epoch information.</DESCRIPTION> 67 79 </FIELD> 68 80 <FIELD name="decStack" arraysize="1" datatype="double" unit="degrees" default="-999"> 69 <DESCRIPTION>Declination mean from stack detections.</DESCRIPTION>81 <DESCRIPTION>Declination from stack detections, weighted mean value across filters, in equinox J2000. See StackObjectThin for stack epoch information.</DESCRIPTION> 70 82 </FIELD> 71 83 <FIELD name="raStackErr" arraysize="1" datatype="float" unit="arcsec" default="-999"> … … 76 88 </FIELD> 77 89 <FIELD name="raMean" arraysize="1" datatype="double" unit="degrees" default="-999"> 78 <DESCRIPTION>Right ascension mean from single epoch detections.</DESCRIPTION>90 <DESCRIPTION>Right ascension from single epoch detections (weighted mean) in equinox J2000 at the mean epoch given by epochMean.</DESCRIPTION> 79 91 </FIELD> 80 92 <FIELD name="decMean" arraysize="1" datatype="double" unit="degrees" default="-999"> 81 <DESCRIPTION>Declination mean from single epoch detections.</DESCRIPTION>93 <DESCRIPTION>Declination from single epoch detections (weighted mean) in equinox J2000 at the mean epoch given by epochMean.</DESCRIPTION> 82 94 </FIELD> 83 95 <FIELD name="raMeanErr" arraysize="1" datatype="float" unit="arcsec" default="-999"> … … 86 98 <FIELD name="decMeanErr" arraysize="1" datatype="float" unit="arcsec" default="-999"> 87 99 <DESCRIPTION>Declination standard deviation from single epoch detections.</DESCRIPTION> 100 </FIELD> 101 <FIELD name="epochMean" arraysize="1" datatype="double" unit="days" default="-999"> 102 <DESCRIPTION>Modified Julian Date of the mean epoch corresponding to raMean, decMean (equinox J2000).</DESCRIPTION> 88 103 </FIELD> 89 104 <FIELD name="posMeanChisq" arraysize="1" datatype="float" unit="dimensionless" default="-999"> … … 140 155 </TABLE> 141 156 <TABLE name="MeanObject"> 142 <DESCRIPTION>Contains the mean photometric information for objects based on the single epoch data, calculated as described in Magnier et al (2013). 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.</DESCRIPTION> 157 158 <DESCRIPTION>Contains the mean photometric information for 159 objects based on the single epoch data, calculated as described 160 in Magnier et al (2013). To be included in this table, an 161 object must be bright enough to have been detected at least once 162 in an individual exposure. PSF, Kron (1980), and aperture 163 magnitudes and statistics are listed for all filters. 164 References: Kron, R. G. 1980, ApJS, 43, 305; Magnier, E. A., 165 Schlafly, E., Finkbeiner, D., et al. 2013, ApJS, 205, 166 20.</DESCRIPTION> 167 143 168 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 144 169 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> -
trunk/ippToPsps/config/tables.P2.vot
r38933 r39081 4 4 <RESOURCE> 5 5 <TABLE name="FrameMeta"> 6 <DESCRIPTION>Contains metadata related to an individual 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.</DESCRIPTION> 6 <DESCRIPTION>Contains metadata related to an individual 7 exposure. A "Frame" refers to the collection of all images 8 obtained by the 60 OTA devices in the camera in a single 9 exposure. The camera configuration, telescope pointing, 10 observation time, and astrometric solution from the detector 11 focal plane (L,M) to the sky (RA,Dec) is provided.</DESCRIPTION> 7 12 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 8 13 <FIELD name="frameID" arraysize="1" datatype="int" unit="dimensionless" default="NA"> … … 158 163 </TABLE> 159 164 <TABLE name="ImageMeta"> 160 <DESCRIPTION>Contains metadata related to an individual OTA image that comprises a portion of the full exposure. The characterization of the image quality, the detrends applied, and the astrometric solution from the raw pixels (X, y) to the detector focal plane (L,M) is provided.</DESCRIPTION>165 <DESCRIPTION>Contains metadata related to an individual OTA image that comprises a portion of the full exposure. The characterization of the image quality, the detrends applied, and the astrometric solution from the raw pixels (X,Y) to the detector focal plane (L,M) is provided.</DESCRIPTION> 161 166 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 162 167 <FIELD name="imageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 167 172 </FIELD> 168 173 <FIELD name="ccdID" arraysize="1" datatype="short" unit="dimensionless" default="NA"> 169 <DESCRIPTION>OTA identifier based on location in the focal plane .</DESCRIPTION>174 <DESCRIPTION>OTA identifier based on location in the focal plane, specific to an individual device.</DESCRIPTION> 170 175 </FIELD> 171 176 <FIELD name="photoCalID" arraysize="1" datatype="int" unit="dimensionless" default="NA"> … … 387 392 </TABLE> 388 393 <TABLE name="Detection"> 389 <DESCRIPTION>Contains single epoch photometry of individual detections . The identifiers connecting the detection 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.</DESCRIPTION>394 <DESCRIPTION>Contains single epoch photometry of individual detections from a single exposure. The identifiers connecting the detection 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.</DESCRIPTION> 390 395 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 391 396 <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 568 573 </TABLE> 569 574 <TABLE name="ImageDetEffMeta"> 570 <DESCRIPTION>Contains the detection efficiency information for a given individual OTA 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>575 <DESCRIPTION>Contains the detection efficiency information for a given individual OTA image. Provides the number of recovered sources out of 500 injected fake source and statistics about the magnitudes of the recovered sources for a range of magnitude offsets.</DESCRIPTION> 571 576 <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM> 572 577 <FIELD name="imageID" arraysize="1" datatype="long" unit="dimensionless" default="NA"> … … 578 583 <FIELD name="magref" arraysize="1" datatype="float" unit="magnitudes" default="NA"> 579 584 <DESCRIPTION>Detection efficiency reference magnitude.</DESCRIPTION> 585 </FIELD> 586 <FIELD name="nInjected" arraysize="1" datatype="int" unit="dimensionless" default="NA"> 587 <DESCRIPTION>Number of fake sources injected in each magnitude bin.</DESCRIPTION> 580 588 </FIELD> 581 589 <FIELD name="offset01" arraysize="1" datatype="float" unit="magnitudes" default="NA"> -
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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