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Changes between Version 640 and Version 641 of MD.GR0


Ignore:
Timestamp:
Feb 6, 2013, 6:37:19 PM (13 years ago)
Author:
Mark Huber
Comment:

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  • MD.GR0

    v640 v641  
    18091809
    18101810
    1811 || [[Image(MD09.GR0.20120601-MD09.deeptest.20120727.s055-MD09.refstack.20120831.s055.i.expfwhm.png,300px)]]  || [[(Image(md09deep_inputtargetfwhm_i.log_fwhmhistomap.png,300px)]] ||
    1812  * (left)
    1813  * (right)
     1811|| [[Image(MD09.GR0.20120601-MD09.deeptest.20120727.s055-MD09.refstack.20120831.s055.i.expfwhm.png,300px)]]  || [[Image(md09deep_inputtargetfwhm_i.log_fwhmhistomap.png,300px)]] ||
     1812 * (left) Sample histogram of the available exposures by camera FWHM_MAJOR in i-band (red) and selected to attempt a deepstack with (blue) in top row, refstack in bottom row.
     1813 * (right) Sample histograms for each skycell over the FPA by FWHM of the input warps in the i-band (blue) and rejected for poor PSF (red). The black dotted line is the input cut @7.5 pixels and the red line is the FWHM_mean+1.5*FWHM_SIGMA additional cut on the input FWHM that is often ~6 pixels given the available input warps -- initially set in an attempt to restrict the target PSF of the convolved version of the stack to ~1.5" but other problem(s) still exist that drive the target PSF much larger.
    18141814
    18151815Stack photometry plots from the Durham 2012 meeting had many faults from bugs in the code, the plots have been updated and include comparison to the ubercal reference catalog