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Changeset 25597


Ignore:
Timestamp:
Sep 27, 2009, 10:41:33 AM (17 years ago)
Author:
eugene
Message:

add some notes

File:
1 edited

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  • branches/eam_branches/20090715/psphot/doc/notes.txt

    r21164 r25597  
     1
     22009.09.26
     3
     4  Remaining PSPHOT Issues:
     5
     6  o soften errors a bit for bright stars?  (essentially allow a
     7    systematic error on the flat of some percentage).  this may help
     8    the very saturated stars (peaks > 10k) which seem to be
     9    excessively driven by the cores.
     10    ** did not seem to be a big success --> makes things worse for f =
     11    0.01, about the same for f = 0.005
     12
     13  * clean up and remove test bits of code.
     14
     15  * clean up psphot.config files : drop unused, fix some conflicting
     16    names, reduce camera-specific options, make S/N limits
     17    consistent...
     18
     19  * EXT fail fit?  lack of iterations?
     20
     21  * extended source output
     22
     23  * still some concerns with the source size analysis: the parameters
     24    space seems fine (Mxx, Myy, nSigma), but we need to define more
     25    sophisticated boundaries (perhaps include dMag or Mag). 
     26
     27  * some optimization issues:         
     28    * too many re-calculations of all magnitude / aperture data
     29    * is FluxScale really faster?  do we need a finer mapping? (5x5
     30      clearly yields too much scatter)
     31
     32  * very saturated stars are somewhat segmented.
     33
     34  * is the residual map failing to be masked at the radius?
     35
     36  * PSF 2D convergence : how to choose between marginally different
     37    options?  (note that the GPC1 images may go to 2x2 instead of 3x3)
     38
     39  * -visual needs more fine-grained control
     40
     41  * visualization graphs should reset the sections in general.
     42
     43  * some excess verbosity (my log level is 9, lower?)
     44
     45  -----
     46
     47  Apparently I'm getting bad psf vs ap mags because of the difference
     48  between linear and non-linear fits.  I think this is due to the
     49  weighting schemes:
     50
     51  psphotChoosePSF & psphotBlendFit depend on POISSON.ERRORS.PHOT.LMM,
     52  which is set to TRUE => use Poisson errors
     53
     54  psphotFitSourcesLinear depends on CONSTANT_PHOTOMETRIC_WEIGHTS,
     55  which is set to TRUE => do not use Poisson errors.
     56
     57  nothing seems to use the value POISSON.ERRORS.PHOT.LIN
     58
     59  ** Poisson errors seeem to be working much better than Constant
     60     errors (as judged by consistency between PSF and APERTURE
     61     magnitdues).  Not sure I understand this.  It could be that the
     62     implementation of Constant errors in the linear fitting analysis
     63     is busted. 
     64
     65  ** Also, I was getting some additional scatter from the FluxScale
     66     (lookup-table for Io -> mags). 
     67
     68     * surprisingly, it is not clear that the FluxScale method is
     69       faster than the more accurate integration technique...
     70
     712009.09.25
     72
     73  Notes on pmSourceMagnitudes:
     74
     75  * in psphotChoosePSF, in pmPSFtry: raw PSF & raw AP
     76  * in psphotChoosePSF, psphotMakeGrowthCurve: uses direct all to pmSourcePhotometryAper
     77  * in psphotSourceSize, in psphotSourceSizePSF, raw PSF & raw AP (but uses moments->Sum) for PSF stars
     78    NOTE: on the initial call, the PSF stars may have had multiple models tried and the psfMag
     79    may not be the value for the chosen model. 
     80  * in psphotSourceSize, in psphotSourceClassRegion, raw PSF & raw AP for all sources for which size is not yet measured.
     81  * in psphotApResid: raw PSF & raw AP for STARS only
     82  * in psphotMagnitudes; corrected PSF & AP mags
    183
    2842009.01.24
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