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Changes between Version 2 and Version 3 of IPP_Progress_Report_20091005


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Timestamp:
Oct 11, 2009, 4:27:39 PM (17 years ago)
Author:
eugene
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  • IPP_Progress_Report_20091005

    v2 v3  
    55
    66=== Eugene Magnier ===
     7
     8This week, my goal was to start the re-processing of data taken in Run 3 & Run 4 with the upgrades to stacking, photometry, including the flat-field correction & y-band fringe corrections.  Although we have had enough tests of the upgraded processing, work has been going a bit slower than hoped on the two detrend issues (flat-field and y-band fringes).  While these were being worked on, we have been running more processing of data that had been collected just before the end of Run 4.  This included a complete sweep through the 'SVS' data (the MOPS ecliptic-plane r-band data), with detections shipped to MOPS Tuesday and Wednesday.  We also have processed the MD and M31 data taken in the last week before the shutdown.
     9
     10On my side, I've been working on the flat-field correction analysis.  Last weekend, I had processed the images taken for the flat-field correction.  However, over the summer we re-organized part of the pipeline to better handle the DVO ingest process, defining a new 'addstar' analysis stage.  I needed to make some changes to the flat-field correction analysis system to interact with this new addstar system, and I also found some errors in the implementation of the addstar stages.  I also updated the flat-field correction system to distinguish between an analysis to generate a flat-field correction and one which tests the flat-field correction (these have slightly different behavior on completion).  We now have flat-field corrections for gizy, and corresponding corrected flats for Run 3 & Run 4, and I have run the tests using those flats on the input data sets (still running as of Sunday 4pm).  The r-band data is waiting for me to fix a minor logic error in the analysis database queries.
    711
    812=== Heather Flewelling ===