Changeset 4896
- Timestamp:
- Aug 29, 2005, 8:42:41 AM (21 years ago)
- Location:
- trunk/doc/psphot
- Files:
-
- 2 added
- 1 edited
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psphot-flow.sxi (added)
-
psphot.tex (added)
-
psphot.txt (modified) (2 diffs)
Legend:
- Unmodified
- Added
- Removed
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trunk/doc/psphot/psphot.txt
r4377 r4896 3 3 4 4 - background 5 6 - discuss dophot, sextractor, daophot 7 - other photometry solutions? 5 8 6 9 - process … … 23 26 - aperture correction 24 27 28 - aperture photometry vs psf photometry 29 30 - aperture is always the reference 31 - how do we choose an appropriate aperture 32 - how do we measure the aperture correction? 33 - predicting / correcting for aperture loss? 34 25 35 - apply PSF to sources 26 36 27 - use fit resultto select PSF-like objects37 - use dsigma to select PSF-like objects 28 38 - fit and subtract PSF-like objects 29 39 40 - fit non-stellar objects 30 41 31 - aperture photometry vs psf photometry 42 - galaxy models 43 - asteroid models 44 - low S/N limits 32 45 33 - aperture is always the reference 34 - how do we choose an appropriate aperture 35 - 46 - user's guide 47 48 - configuration parameters 49 - input images / output files 50 - command-line arguments 51 52 - demonstration tests 53 54 - simulated data 55 - astrometric accuracy 56 - as a function of S/N 57 - as a function of crowding 58 - as a function of fringe residual amplitude & scale 59 - as a function of PSF model quality 60 - as a function of seeing 61 - photometric accuracy 62 - as a function of S/N 63 - as a function of crowding 64 - as a function of fringe residual amplitude & scale 65 - as a function of seeing 66 - as a function of PSF model quality 67 - real data 68 - quality of galaxy models 69 - accuracy of PSF models (megacam, cfh12k, suprime, skyprobe?) 70
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