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Changes between Version 9 and Version 10 of IPP_Progress_Report_20100419


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Timestamp:
Apr 26, 2010, 5:01:31 PM (16 years ago)
Author:
eugene
Comment:

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  • IPP_Progress_Report_20100419

    v9 v10  
    55
    66=== Eugene Magnier ===
     7
     8We have largely been working to iron out wrinkles and issues as they come up, with special effort on the overall detection efficiency.  We've been interacting a lot in the past 2-3 weeks with the MOPS team, and finding a number of interesting issues.  Paul has been worrying about the most important of these: an error in the covariance calculation which was preventing the diff detection from reaching as deep as it should have been.  With that error identified and corrected (as well as a related error in warp due to the change of pixel scale), he has been trying to understand the impact of the fix on the magic masking.  We will need to iterate with Paul Sydney for final validation, but we can test the magic impact with the magic verification data set used before the start of Demo month.  It may be necessary to tweak the magic threshold to reach the right balance between excess streaks and catching all real ones.
     9
     10I spent a couple of days this week on the IfA TAC, which takes a lot of time (and mental energy).  After that I've been working on the extended source photometry.  This has been dormant for some months, but I've brought it back to life.  I have updated the output functions to save the radial surface brightness measurements, with options to make it match the SDSS analysis.  I am running tests on SDSS image to compare the psphot measurements with SDSS measurements of the same pixels.  After these tests are done, it should not be hard to turn on this analysis in the 5-way image mode.
    711
    812=== Heather Flewelling ===