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Changes between Version 10 and Version 11 of IPP_Progress_Report_20120903


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Timestamp:
Sep 11, 2012, 1:20:08 PM (14 years ago)
Author:
eugene
Comment:

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  • IPP_Progress_Report_20120903

    v10 v11  
    66=== Eugene Magnier ===
    77
     8 * finished up the psphot saturated star radial profile analysis, and it really helps a lot (see Bill's report).  Also fixed some issues with duplicate detections (using a mask to block re-detection of the cores) and negative fluxes in linear fits (at least in psphot; psphotStack was fixed earlier).
     9 * update the dvo schema and pushed changes into the trunk.
     10
    811=== Serge Chastel ===
    912 * Tuesday off
    1013 * Documentation of the "Who is the cluster?" software.
    1114 * "Who is the cluster?" given to MOPS/Denver.
     15
    1216=== Heather Flewelling ===
    1317
     
    2125   * attempts at processing isp-sas stuff is located here: http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/IspSasProcessing
    2226 * lots of sciency stuff with JT (not involving sas! )
     27
    2328=== Mark Huber ===
    2429 * vacation
     30
    2531=== Bill Sweeney ===
    2632 * Tested Gene's improvements to psphotStack to better model massively saturated stars. The number of false detections is greatly reduced around such objects.
     
    3440 * Lot's of assistant czar work helping to manage the fallout from the MHPCC cluster power outage and various other strange problems.
    3541
    36 
    3742=== Chris Waters ===
    3843 * Investigated the possibility of minimizing row-to-row variations by constructing 8 per-OTA correction images.  http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/GPC1_Bias_Pattern_Study This looks somewhat promising, although it will require some level of development.