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Ignore:
Timestamp:
Nov 9, 2015, 3:19:48 PM (11 years ago)
Author:
watersc1
Message:

Fix table descriptions that were line-broken.

File:
1 edited

Legend:

Unmodified
Added
Removed

  • trunk/ippToPsps/config/tables.ST.vot

    r39081 r39088  
    66    <!-- StackMeta Table ************************************************** -->
    77    <TABLE name="StackMeta">
    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>
     8      <DESCRIPTION>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.</DESCRIPTION>
    139      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>             
    1410      <FIELD name="stackImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA">
    … …  
    27002696    <TABLE name="StackApFlxExGalUnc">
    27012697
    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>
     2698      <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.  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.</DESCRIPTION>
    27142699
    27152700      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    … …  
    33353320    <TABLE name="StackApFlxExGalCon6">
    33363321
    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>
     3322      <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).  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.</DESCRIPTION>
    33503323
    33513324      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    … …  
    39723945    <TABLE name="StackApFlxExGalCon8">
    39733946
    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>
     3947      <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).  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.</DESCRIPTION>
    39873948
    39883949      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    … …  
    48694830    <TABLE name="StackDetEffMeta">
    48704831
    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>
     4832      <DESCRIPTION>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.</DESCRIPTION>
    48754833
    48764834      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
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