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Changes between Version 9 and Version 10 of IPP_Progress_Report_20100726


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Timestamp:
Aug 4, 2010, 9:20:34 AM (16 years ago)
Author:
eugene
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  • IPP_Progress_Report_20100726

    v9 v10  
    55
    66=== Eugene Magnier ===
     7
     8I've been splitting my time this week on three areas: extended sources, image subtraction, and dvo database issues.  For extended sources, I have concluded that the current psf-convolved fitting is working fine, but it is too slow for practical work.  There are a couple of things that I can do to speed it up substantially: convert the convolution to use FFTs and add in threading.  Both are fairly straight-forward given the rest of the IPP code. 
     9
     10Meanwhile, I have been looking at cases where the warp-warp subtractions are resulting in high numbers of false positives in an attempt to either characterize the false positives and/or to reduce them up front.  Towards the first goal, I have added the ability to associate the diff detections with the nearest positive source above some S/N limit in both of the input images.  I've added 5 new fields to the output cmf files: the S/N and distance to the source in the positive image (relative to the diff detection) and the same for the negative image, and a new set of flags, including bits the identify that a diff source is matched to a positive image source. 
     11
     12In terms of reducing the false positives, a major contributor seems to come from times when the image quality difference is large (eg, a sub-arcsecond image and one with 1.6 arcsec FWHM).  It seems that at least 2 bad things are happening in ppSub in these cases (and maybe to some extent in less extreme cases): 1) the FWHM-based kernel scaling code saturates at one of the extremes, and 2) the normalization is poorly measured.  I suspect (2) is more of a problem than (1), but both are a concern.  I am looking into improving the robustness of the normalization measurement. 
     13
     14On DVO related issues: I have tested the updated dvomerge code -- I reworked the processing order so that only the new database is completely loaded rather than the output database -- and find that it have a much improved performance.  It now runs at a rate that is essentially linear in the size of the input database (ie, the incoming mini database).  It is still a bit slower than I might want: it runs at a rate equivalent to about 5-10 MByte per second, so it is clearly not I/O limited.  It is single threaded, but it would not be difficult to change to a multi-threaded option (one thread per merged database sky region).
    715
    816=== Serge Chastel ===