- Timestamp:
- Sep 29, 2009, 10:08:18 AM (17 years ago)
- File:
-
- 1 edited
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branches/eam_branches/20090715/ippconfig/recipes/psphot.config
r25657 r25658 53 53 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 54 54 FOOTPRINT_NPIXMIN S32 5 # Minimum size of a pmFootprint 55 FOOTPRINT_NSIGMA_LIMIT F32 20 # threshold for bright pmFootprint detection56 FOOTPRINT_NSIGMA_LIMIT_2 F32 4 # threshold for faint pmFootprint detection57 55 FOOTPRINT_GROW_RADIUS S32 3 # How much to grow bright footprints 58 56 FOOTPRINT_GROW_RADIUS_2 S32 5 # How much to grow faint footprints … … 77 75 SKY_OUTER_RADIUS F32 25 # square annulus for local sky measurement 78 76 PSF_MOMENTS_RADIUS F32 3 # XXX this is now autoscaled 79 PSF_SN_LIM F32 50 # minimum S/N for stars used for PSF model80 PSF_MAX_NSTARS S32 200 # limit number of stars used for PSF model77 PSF_SN_LIM F32 20 # minimum S/N for stars used for PSF model 78 PSF_MAX_NSTARS S32 500 # limit number of stars used for PSF model 81 79 PSF_CLUMP_NSIGMA F32 1.5 # region of Sx,Sy plane to use for selecting PSF stars 82 80 PSF_CLUMP_GRID_SCALE F32 0.2 # size of Sx,Sy image pixel … … 139 137 # this model is used for approximate subtraction in the main object analysis step 140 138 EXT_MODEL STR PS_MODEL_QGAUSS 141 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit142 139 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit 143 140 EXT_FIT_PADDING F32 5 # extra annulus to use for fit
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