Changeset 25597
- Timestamp:
- Sep 27, 2009, 10:41:33 AM (17 years ago)
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branches/eam_branches/20090715/psphot/doc/notes.txt
r21164 r25597 1 2 2009.09.26 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 71 2009.09.25 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 1 83 2 84 2009.01.24
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