Changeset 25756 for trunk/ippconfig/recipes
- Timestamp:
- Oct 2, 2009, 3:13:59 PM (17 years ago)
- Location:
- trunk/ippconfig/recipes
- Files:
-
- 2 edited
-
ppSim.config (modified) (2 diffs)
-
psphot.config (modified) (11 diffs)
Legend:
- Unmodified
- Added
- Removed
-
trunk/ippconfig/recipes/ppSim.config
r24813 r25756 50 50 51 51 STARS.FAKE BOOL TRUE # Add fake stars, randomly distributed? 52 STARS.LUM F32 0. 6# Stellar luminosity function slope (magnitude slope)53 STARS.MAG F32 15.5 # Brightest magnitude for fake stars 54 STARS.DENSITY F32 50.0 # Stellar density (per square degree) at the brightest magnitude52 STARS.LUM F32 0.35 # Stellar luminosity function slope (magnitude slope) 53 STARS.MAG F32 15.5 # Brightest magnitude for fake stars (choose based on real catalog limit) 54 STARS.DENSITY F32 1.0 # Stellar density (per square degree) at the brightest magnitude 55 55 STARS.SIGMA.LIM F32 5.0 # significance of faintest sources 56 56 … … 185 185 END 186 186 187 STACKTEST.MAKE METADATA 188 END 189 190 STACKTEST.RUN METADATA 191 END 192 187 193 # Overrides for creating large holes in the image 188 194 LARGEHOLES METADATA -
trunk/ippconfig/recipes/psphot.config
r25383 r25756 2 2 # these options turn on different inputs and/or outputs 3 3 SAVE.OUTPUT BOOL TRUE 4 SAVE.BACKMDL BOOL FALSE4 SAVE.BACKMDL BOOL TRUE 5 5 SAVE.BACKMDL.STDEV BOOL FALSE 6 6 SAVE.BACKGND BOOL FALSE 7 7 SAVE.BACKSUB BOOL FALSE 8 8 SAVE.RESID BOOL FALSE 9 SAVE.PLOTS BOOL FALSE 9 10 SAVE.PSF BOOL TRUE 10 11 LOAD.PSF BOOL FALSE 11 SAVE.PLOTS BOOL FALSE12 12 13 13 # format for output CMF files … … 15 15 16 16 # the zero point is used to set a basic scale for DVO 17 # XXX it may not currently be read : double check this (EAM) 18 ZERO_POINT F32 25.000 # zero point used by DVO 19 ZERO_PT F32 25.000 # zero point used by DVO 17 ZERO_PT F32 25.000 # zero point used by DVO XXX deprecate this 20 18 21 19 # these parameter govern how the background is measured … … 23 21 BACKGROUND.YBIN S32 128 # size of background superpixels 24 22 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 23 24 # soften the errors for bright pixels: 25 SOFTEN.VARIANCE BOOL FALSE 26 SOFTEN.VARIANCE.FRACTION F32 0.0 25 27 26 28 SKY_BIAS F32 0.0 # offset applied to measured sky (FOR TESTING) … … 43 45 PEAKS_SMOOTH_SIGMA F32 1.0 # smoothing kernel sigma in pixels 44 46 PEAKS_SMOOTH_NSIGMA F32 2.0 # smoothing kernel width in sigmas 45 PEAKS_NSIGMA_LIMIT F32 2 5.0 # peak significance threshold47 PEAKS_NSIGMA_LIMIT F32 20.0 # peak significance threshold 46 48 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold 47 PEAKS_NMAX S32 0 # on first pass, only keep NMAX peaks (0 == all) 48 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_GROW_RADIUS S32 3 # How much to grow bright footprints 56 FOOTPRINT_GROW_RADIUS_2 S32 5 # How much to grow faint footprints 57 FOOTPRINT_CULL_NSIGMA_DELTA F32 4 # Cull peaks that aren't nsigma above coll to neighbour 58 FOOTPRINT_CULL_NSIGMA_MIN F32 1 # Minimum height of colls in units of skyStdev 59 FOOTPRINT_CULL_NSIGMA_PAD F32 0.01 # Fractional Padding for stdev 60 61 # parameter for the simple deblending 62 DEBLEND_PEAK_FRACTION F32 0.1 63 DEBLEND_SKY_NSIGMA F32 10.0 49 64 50 65 # parameters to control the selection of the peak in the Sx,Sy plane 51 66 MOMENTS_SCALE F32 0.25 52 MOMENTS_SN_MIN F32 10.0 # min S/N to measure moments67 MOMENTS_SN_MIN F32 0.0 # min S/N to measure moments (default: measure all objects) 53 68 MOMENTS_SX_MAX F32 50.0 54 69 MOMENTS_SY_MAX F32 50.0 55 70 MOMENTS_AR_MAX F32 1.5 # maximum axial ratio: 1 / AR < (sx / sy) < AR 56 MOMENTS_MIN_PIXEL_SN F32 0.0 # XXX caution on this: too high and we will excessively clip 57 MOMENTS_GAUSS_SIGMA F32 4.0 # XXX TEST THIS: sigma in pixels (should be >> seeing equiv) 71 MOMENTS_GAUSS_SIGMA F32 4.0 # XXX this is now autoscaled 58 72 59 73 # basic object statistics 60 74 SKY_INNER_RADIUS F32 15 # square annulus for local sky measurement 61 75 SKY_OUTER_RADIUS F32 25 # square annulus for local sky measurement 62 PSF_MOMENTS_RADIUS F32 3 # calculate initial source moments with this radius63 PSF_SN_LIM F32 50 # minimum S/N for stars used for PSF model64 PSF_MAX_NSTARS S32 200 # limit number of stars used for PSF model76 PSF_MOMENTS_RADIUS F32 3 # XXX this is now autoscaled 77 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 65 79 PSF_CLUMP_NSIGMA F32 1.5 # region of Sx,Sy plane to use for selecting PSF stars 66 PSF_CLUMP_GRID_SCALE F32 0. 5# size of Sx,Sy image pixel80 PSF_CLUMP_GRID_SCALE F32 0.2 # size of Sx,Sy image pixel 67 81 68 82 PSF_CLUMP_NX S32 1 # subdivide image in to NX x NY regions for … … 80 94 PSF_MODEL STR PS_MODEL_GAUSS 81 95 # PSF_MODEL STR PS_MODEL_PGAUSS 82 # PSF_MODEL STR PS_MODEL_QGAUSS83 # PSF_MODEL STR PS_MODEL_TGAUSS # not well tested, not very successful84 96 85 97 # PSF.TREND.MASK must be a 2D polynomial … … 98 110 PSF.FAKE.ALLOW BOOL FALSE # Allow use of fake PSFs when having trouble? 99 111 100 PSF_FIT_RADIUS F32 15.0 # fitting radius for test PSF model112 PSF_FIT_RADIUS F32 15.0 # XXX this is now autoscaled 101 113 PSF_REF_RADIUS F32 25.0 # aperture magnitudes are scaled via 102 # curve-of-growth to this radius 114 # curve-of-growth to this radius 115 116 PSF_FIT_RADIUS_SCALE F32 7.0 # fitting radius for test PSF model 117 PSF_APERTURE_SCALE F32 4.5 # fitting radius for test PSF model 118 103 119 # PSF-like source model parameters 104 120 PSF_FIT_NSIGMA F32 1.0 # significance for pixel included in fit 105 121 PSF_FIT_PADDING F32 2.0 # extra annulus to use for fit 106 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation107 122 PSF_MIN_SN F32 2.0 # reject objects below this significance 108 PSF_MAX_CHI F32 50.0 # reject objects worse tha tthis123 PSF_MAX_CHI F32 50.0 # reject objects worse than this 109 124 FULL_FIT_SN_LIM F32 50.0 110 125 … … 117 132 PSF.RESIDUALS.STATISTIC STR ROBUST_MEDIAN # statistic to use for generating the residual 118 133 PSF.RESIDUALS.SPATIAL_ORDER S32 0 # fit spatial variations of the residuals at this order (0,1) 119 PSF.RESIDUALS.PIX.SN F32 5.0 # keep this pixel if residual is more significant than this 134 PSF.RESIDUALS.PIX.SN F32 0.0 # keep this pixel if residual is more significant than this 135 PSF.RESIDUALS.RADIUS F32 8.0 # keep this pixel if residual is more significant than this 120 136 121 137 # this model is used for approximate subtraction in the main object analysis step 122 138 EXT_MODEL STR PS_MODEL_QGAUSS 123 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit124 139 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit 125 140 EXT_FIT_PADDING F32 5 # extra annulus to use for fit 126 141 EXT_MOMENTS_RADIUS F32 31 142 EXT_FIT_MAX_RADIUS F32 128 # non-sensical to fit objects larger than the background mesh 127 143 128 144 EXT_FIT_ITER S32 20 # Maximum number of fitting iterations for EXT … … 172 188 PETROSIAN_FLUX_RATIO F32 0.1 # we measure out to where flux = R0 * FLUX_RATIO 173 189 174 FITMODE STR BLEND175 DEBLEND_PEAK_FRACTION F32 0.1176 DEBLEND_SKY_NSIGMA F32 10.0177 178 190 # APTREND STR NONE, CONSTANT, SKYBIAS, SKYSAT, XY_LIN, SKY_XY_LIN, SKYSAT_XY_LIN, ALL 179 MEASURE.APTREND BOOL FALSE ### Gene says there's bugs in this part191 MEASURE.APTREND BOOL TRUE 180 192 APTREND STR CONSTANT 181 AP_MIN_SN F32 25.0193 AP_MIN_SN F32 0.0 # measure apMags for all sources by default 182 194 APTREND.NSTAR.MIN S32 5 183 195 APTREND.ORDER.MAX S32 5 … … 196 208 197 209 IGNORE_GROWTH BOOL FALSE 198 CONSTANT_PHOTOMETRIC_WEIGHTS BOOL TRUE # Should the photometric code [currently only ensemblePSF] refuse to weight each pixel by it's significance?210 CONSTANT_PHOTOMETRIC_WEIGHTS BOOL FALSE 199 211 INTERPOLATE_AP BOOL TRUE 200 212 … … 207 219 NOISE.FACTOR F32 5.0 208 220 NOISE.SIZE F32 2.0 209 210 USE_FOOTPRINTS BOOL F # use new pmFootprint peak packaging211 FOOTPRINT_NPIXMIN S32 5 # Minimum size of a pmFootprint212 FOOTPRINT_NSIGMA_LIMIT F32 20 # threshold for bright pmFootprint detection213 FOOTPRINT_NSIGMA_LIMIT_2 F32 4 # threshold for faint pmFootprint detection214 FOOTPRINT_GROW_RADIUS S32 3 # How much to grow bright footprints215 FOOTPRINT_GROW_RADIUS_2 S32 5 # How much to grow faint footprints216 FOOTPRINT_CULL_NSIGMA_DELTA F32 4 # Cull peaks that aren't nsigma above coll to neighbour217 FOOTPRINT_CULL_NSIGMA_MIN F32 1 # Minimum height of colls in units of skyStdev218 FOOTPRINT_CULL_NSIGMA_PAD F32 0.01 # Fractional Padding for stdev219 221 220 222 # alternate PSPHOT-type recipes … … 261 263 262 264 PSPHOT.CR.NSIGMA.LIMIT F32 3.0 # sources with crNsigma greater that this get tagged as likely cosmic rays 263 PSPHOT.EXT.NSIGMA.LIMIT F32 4.0 # sources with extNsigma greater that this get tagged as likely extended sources 265 PSPHOT.EXT.NSIGMA.LIMIT F32 3.0 # sources with extNsigma greater that this get tagged as likely extended sources 266 PSPHOT.EXT.NSIGMA.MOMENTS F32 2.0 # sources with extNsigma greater that this get tagged as likely extended sources 264 267 PSPHOT.CR.GROW S32 1 # Number of pixels to grow CR mask 265 268 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights
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