Changeset 25657
- Timestamp:
- Sep 29, 2009, 9:39:48 AM (17 years ago)
- File:
-
- 1 edited
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branches/eam_branches/20090715/ippconfig/recipes/psphot.config
r25656 r25657 15 15 16 16 # the zero point is used to set a basic scale for DVO 17 ZERO_PT F32 25.000 # zero point used by DVO 17 ZERO_PT F32 25.000 # zero point used by DVO XXX deprecate this 18 18 19 19 # these parameter govern how the background is measured … … 45 45 PEAKS_SMOOTH_SIGMA F32 1.0 # smoothing kernel sigma in pixels 46 46 PEAKS_SMOOTH_NSIGMA F32 2.0 # smoothing kernel width in sigmas 47 PEAKS_NSIGMA_LIMIT F32 2 5.0 # peak significance threshold47 PEAKS_NSIGMA_LIMIT F32 20.0 # peak significance threshold 48 48 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold 49 PEAKS_NMAX S32 0 # on first pass, only keep NMAX peaks (0 == all) 50 PEAKS_MIN_GAUSS F32 0.5 # Minimum valid fraction of kernel 49 PEAKS_NMAX S32 5000 # on first pass, only keep NMAX peaks (0 == all) 50 PEAKS_MIN_GAUSS F32 0.5 # On quick convolution, mask pixels for which the 51 # input pixels contribute less than this fraction of the flux 52 # parameters which adjust the footprint analysis 53 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 54 FOOTPRINT_NPIXMIN S32 5 # Minimum size of a pmFootprint 55 FOOTPRINT_NSIGMA_LIMIT F32 20 # threshold for bright pmFootprint detection 56 FOOTPRINT_NSIGMA_LIMIT_2 F32 4 # threshold for faint pmFootprint detection 57 FOOTPRINT_GROW_RADIUS S32 3 # How much to grow bright footprints 58 FOOTPRINT_GROW_RADIUS_2 S32 5 # How much to grow faint footprints 59 FOOTPRINT_CULL_NSIGMA_DELTA F32 4 # Cull peaks that aren't nsigma above coll to neighbour 60 FOOTPRINT_CULL_NSIGMA_MIN F32 1 # Minimum height of colls in units of skyStdev 61 FOOTPRINT_CULL_NSIGMA_PAD F32 0.01 # Fractional Padding for stdev 62 63 # parameter for the simple deblending 64 DEBLEND_PEAK_FRACTION F32 0.1 65 DEBLEND_SKY_NSIGMA F32 10.0 51 66 52 67 # parameters to control the selection of the peak in the Sx,Sy plane … … 176 191 PETROSIAN_FLUX_RATIO F32 0.1 # we measure out to where flux = R0 * FLUX_RATIO 177 192 178 FITMODE STR BLEND179 DEBLEND_PEAK_FRACTION F32 0.1180 DEBLEND_SKY_NSIGMA F32 10.0181 182 193 # APTREND STR NONE, CONSTANT, SKYBIAS, SKYSAT, XY_LIN, SKY_XY_LIN, SKYSAT_XY_LIN, ALL 183 194 MEASURE.APTREND BOOL TRUE … … 211 222 NOISE.FACTOR F32 5.0 212 223 NOISE.SIZE F32 2.0 213 214 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging215 FOOTPRINT_NPIXMIN S32 5 # Minimum size of a pmFootprint216 FOOTPRINT_NSIGMA_LIMIT F32 20 # threshold for bright pmFootprint detection217 FOOTPRINT_NSIGMA_LIMIT_2 F32 4 # threshold for faint pmFootprint detection218 FOOTPRINT_GROW_RADIUS S32 3 # How much to grow bright footprints219 FOOTPRINT_GROW_RADIUS_2 S32 5 # How much to grow faint footprints220 FOOTPRINT_CULL_NSIGMA_DELTA F32 4 # Cull peaks that aren't nsigma above coll to neighbour221 FOOTPRINT_CULL_NSIGMA_MIN F32 1 # Minimum height of colls in units of skyStdev222 FOOTPRINT_CULL_NSIGMA_PAD F32 0.01 # Fractional Padding for stdev223 224 224 225 # alternate PSPHOT-type recipes
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