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Changes between Version 37 and Version 38 of MD_WSdiffim_photcheck_test20121004


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Timestamp:
Nov 15, 2012, 10:56:54 AM (14 years ago)
Author:
Mark Huber
Comment:

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  • MD_WSdiffim_photcheck_test20121004

    v37 v38  
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    58 Manually rerunning WSdiffims with more current ipp-20121026/trunk tag (conv + unconv refstack):
     58Manually rerunning WSdiffims:
     59 * conv direction correct (default is conv refstack)? Yes according the inputs from ppSub logs (conv refstack only, unconv better by ~1 pixel), and Kron R measure appears similar to SMF PSF size.
     60{{{
     61---- o6157g0218o
     62      Input FWHM: 9.713536
     63      Reference FWHM: 4.809747
     64        Kron Radii vs FWHMs 1: fwhm: 9.713536, kron 7.794752
     65        Kron Radii vs FWHMs 2: fwhm: 4.809747, kron 4.897604
     66---- o6157g0219o
     67      Input FWHM: 9.825516
     68      Reference FWHM: 4.809747
     69        Kron Radii vs FWHMs 1: fwhm: 9.825516, kron 7.951603
     70        Kron Radii vs FWHMs 2: fwhm: 4.809747, kron 4.905538
     71
     72}}}
     73
     74 * with more current ipp-20121026/trunk tag (conv + unconv refstack):
    5975{{{
    6076IPP_IDET  CAL_PSF_MAG  CAL_PSF_MAG_SIG  PSF_INST_MAG  PSF_INST_MAG_SIG  AP_MAG  PSF_MAJOR  PSF_QF_PERFECT  FLAGS  FLAGS2  DIFF_NRATIO_BAD  rsep
     
    6884}}}
    6985
    70 Manually rerunning WSdiffims (conv) with tag ipp-20110622 that was active when photometry looked better last year (see example mag plot for TNO145452 below):
     86 * with older ipp-20110622 tag (conv only) that was active when photometry "looked better" last year (see example mag plot for TNO145452 below):
    7187{{{
    7288