IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Changeset 39088 for trunk


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

Fix table descriptions that were line-broken.

Location:
trunk/ippToPsps/config
Files:
7 edited

Legend:

Unmodified
Added
Removed

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

    r39083 r39088  
    55    <TABLE name="DiffMeta">
    66
    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>
     7      <DESCRIPTION>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.</DESCRIPTION>
    138
    149      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>           
    … …  
    3227      </FIELD>
    3328      <FIELD name="posImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA">
    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>
     29        <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>
    3530      </FIELD>
    3631      <FIELD name="negImageID" arraysize="1" datatype="long" unit="dimensionless" default="NA">

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

    r39081 r39088  
    44  <RESOURCE>
    55    <TABLE name="ForcedMeanObject">
    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>
     6      <DESCRIPTION>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.</DESCRIPTION>
    187      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    198      <FIELD name="objID" arraysize="1" datatype="long" unit="dimensionless" default="NA">

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

    r39081 r39088  
    126126    <TABLE name="ForcedWarpMeasurement">
    127127
    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>
     128      <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>
    135129
    136130      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>

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

    r39087 r39088  
    2323    </TABLE>
    2424    <TABLE name="FitModel">
    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>
     25      <DESCRIPTION>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.</DESCRIPTION>
    3126      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    3227      <FIELD name="fitModelID" arraysize="1" datatype="short">

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

    r39081 r39088  
    55    <TABLE name="ObjectThin">
    66
    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>
     7      <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 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.</DESCRIPTION>
    188
    199      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    … …  
    156146    <TABLE name="MeanObject">
    157147
    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>
     148      <DESCRIPTION>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.</DESCRIPTION>
    167149
    168150      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>

  • trunk/ippToPsps/config/tables.P2.vot

    r39081 r39088  
    44  <RESOURCE>
    55    <TABLE name="FrameMeta">
    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>
     6      <DESCRIPTION>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.</DESCRIPTION>
    127      <PARAM arraysize="1" datatype="char" ucd="meta.bib.author" name="Author" value="PSPS"></PARAM>
    138      <FIELD name="frameID" arraysize="1" datatype="int" unit="dimensionless" default="NA">

  • 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>
Note: See TracChangeset for help on using the changeset viewer.