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Changes between Version 8 and Version 9 of IPP_Progress_Report_20121015


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Timestamp:
Oct 24, 2012, 8:43:06 AM (14 years ago)
Author:
eugene
Comment:

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  • IPP_Progress_Report_20121015

    v8 v9  
    44(Up to [wiki:IPP_Progress_Reports IPP Progress Reports])
    55
    6 === Eugene Magnier ===
     6=== Eugene Magnier ==='
     7
     8 * investigations in to more ipp / psps concerns (PSF theta - found a bug in the I/O layer treating degrees as radians, funny kron mags noted by Ken - these were known garbage based on dvo / psps flags)
     9 * some exploration of the PS and PS1SC web sites and content management systems.  Make a mock-up of the PS public web site using Word Press that is not bad, but would need some cleanup.
     10 * work on the IPP data distribution pages, need to make these a bit more clear
     11 * readying phot ladder paper for submission.
    712
    813=== Serge Chastel ===
     
    1015 * Spent (wasted?) more time than I wanted with Condor web services compilation/installation at mhpcc for the ippdor account;
    1116 * mops data format 3 tests preparation;
     17
    1218=== Heather Flewelling ===
    1319
     
    1622 * ipptopsps work
    1723 * some science stuff
     24
    1825=== Mark Huber ===
    1926  * various liaison issues
    2027  * MD05 prep for full reprocessing of all exposures that were not done with the ubercal catalog
    2128  * observing at subaru
     29
    2230=== Bill Sweeney ===
    2331 * Continued investigation into the differences between the psphotStack aperture flux measurements for the different convolved images. It appears that we have different flux level when we build the psf matched stack. For a given radial aperture, the difference is .02 - .04 magnitudes where the image convolved to 6 pixels is higher. The offset is a function of the stack_id. The cause is still under investigation