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Changes between Version 133 and Version 134 of ppSub_testing_201201


Ignore:
Timestamp:
May 24, 2012, 11:14:58 PM (14 years ago)
Author:
Mark Huber
Comment:

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  • ppSub_testing_201201

    v133 v134  
    838838
    839839 * 1: MD04 Skycell V3.084 MJD 56031 z-band http://star.pst.qub.ac.uk/ps1/psdb/candidate/1100018991032613300/
    840  * 2: MD07 Skycell V3.031 MJD 55742 z-band http://star.pst.qub.ac.uk/ps1/psdb/candidate/1141453871521649300/ -- V2 requested, not setup to redo so will only do the i-band in the set
     840 * 2: MD07 Skycell V3.031 MJD 55742 z-band http://star.pst.qub.ac.uk/ps1/psdb/candidate/1141453871521649300/
     841   * V2 specifically requested, but not setup to redo these old format/data. Will only do the i-band V3 in the set.
    841842 * 3: MD04 Skycell V3.035 MJD 56027 i-band http://star.pst.qub.ac.uk/ps1/psdb/candidate/1095825621012824500/
    842843 * 4: MD07 Skycell V3.041 MJD 56000 g-band http://star.pst.qub.ac.uk/ps1/psdb/candidate/1142317691530726200/
     
    874875
    875876Diffims are not necessarily better for convolving the other direction. More often than not seems the psphot detections of the source of interest is dropped from the inverting of the core flux, but not for all detections.
     877Diffims are not necessarily better for convolving the other direction. More often than not seems the psphot detections of the source of interest is dropped from the inverting of the core flux, but not for all detections.