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Changes between Version 13 and Version 14 of DVO_TopLevel


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Timestamp:
May 8, 2012, 3:07:45 PM (14 years ago)
Author:
heather
Comment:

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  • DVO_TopLevel

    v13 v14  
    2121
    2222The standard implementation of DVO uses a stores the database information as a collection FITS tables.  For a subset of the tables (Average, SecFilt, Measure, Missing), the data is partitioned into multiple files representing different regions on the sky.  The partitioning scheme allows for a wide range of scale on which the sky is divided.  At one extreme, the entire sky is represented by a single file.  At the next level, this is split into Declination bands of width 7.5 degrees.  Next, these bands are split into RA ranges.  The next levels subdivide the RA / DEC ranges into smaller and smaller patches.  From the third level on down, the size of the sky regions varies with Galactic latitude to better sample regions of high and low stellar density.
     23
     24 more information on dvo databases:
     25
     26 * [wiki:DVO_format format of dvodb files]
     27 * [wiki:DVO_SkyTable layout of dvodb files]
    2328
    2429=== DVO Shell ===