- Timestamp:
- May 3, 2010, 8:50:52 AM (16 years ago)
- Location:
- branches/simtest_nebulous_branches
- Files:
-
- 3 edited
Legend:
- Unmodified
- Added
- Removed
-
branches/simtest_nebulous_branches
- Property svn:mergeinfo changed
-
branches/simtest_nebulous_branches/ippconfig
-
Property svn:mergeinfo
set to (toggle deleted branches)
/trunk/ippconfig merged eligible /branches/eam_branches/stackphot.20100406/ippconfig 27624-27656 /branches/pap_delete/ippconfig 27530-27595
-
Property svn:mergeinfo
set to (toggle deleted branches)
-
branches/simtest_nebulous_branches/ippconfig/recipes/psphot.config
r24879 r27840 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 72 73 # calculate difference stats? 74 DIFF_STATS BOOL FALSE 58 75 59 76 # basic object statistics 60 77 SKY_INNER_RADIUS F32 15 # square annulus for local sky measurement 61 78 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 model79 PSF_MOMENTS_RADIUS F32 3 # XXX this is now autoscaled 80 PSF_SN_LIM F32 20 # minimum S/N for stars used for PSF model 81 PSF_MAX_NSTARS S32 500 # limit number of stars used for PSF model 65 82 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 pixel83 PSF_CLUMP_GRID_SCALE F32 0.2 # size of Sx,Sy image pixel 67 84 68 85 PSF_CLUMP_NX S32 1 # subdivide image in to NX x NY regions for … … 80 97 PSF_MODEL STR PS_MODEL_GAUSS 81 98 # 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 99 85 100 # PSF.TREND.MASK must be a 2D polynomial … … 98 113 PSF.FAKE.ALLOW BOOL FALSE # Allow use of fake PSFs when having trouble? 99 114 100 PSF_FIT_RADIUS F32 15.0 # fitting radius for test PSF model115 PSF_FIT_RADIUS F32 15.0 # XXX this is now autoscaled 101 116 PSF_REF_RADIUS F32 25.0 # aperture magnitudes are scaled via 102 # curve-of-growth to this radius 117 # curve-of-growth to this radius 118 119 PSF_FIT_RADIUS_SCALE F32 7.0 # fitting radius for test PSF model 120 PSF_APERTURE_SCALE F32 4.5 # fitting radius for test PSF model 121 103 122 # PSF-like source model parameters 104 123 PSF_FIT_NSIGMA F32 1.0 # significance for pixel included in fit 105 124 PSF_FIT_PADDING F32 2.0 # extra annulus to use for fit 106 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation107 125 PSF_MIN_SN F32 2.0 # reject objects below this significance 108 PSF_MAX_CHI F32 50.0 # reject objects worse tha tthis126 PSF_MAX_CHI F32 50.0 # reject objects worse than this 109 127 FULL_FIT_SN_LIM F32 50.0 110 128 … … 117 135 PSF.RESIDUALS.STATISTIC STR ROBUST_MEDIAN # statistic to use for generating the residual 118 136 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 137 PSF.RESIDUALS.PIX.SN F32 0.0 # keep this pixel if residual is more significant than this 138 PSF.RESIDUALS.RADIUS F32 8.0 # keep this pixel if residual is more significant than this 120 139 121 140 # this model is used for approximate subtraction in the main object analysis step 122 141 EXT_MODEL STR PS_MODEL_QGAUSS 123 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit124 142 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit 125 143 EXT_FIT_PADDING F32 5 # extra annulus to use for fit 126 144 EXT_MOMENTS_RADIUS F32 31 145 EXT_FIT_MAX_RADIUS F32 128 # non-sensical to fit objects larger than the background mesh 127 146 128 147 EXT_FIT_ITER S32 20 # Maximum number of fitting iterations for EXT … … 132 151 EXTENDED_SOURCE_ANALYSIS BOOL FALSE # perform any of the aperture-like measurements? 133 152 EXTENDED_SOURCE_SN_LIM F32 20.0 153 EXTENDED_SOURCE_RAW_RADIUS BOOL FALSE 134 154 EXTENDED_SOURCE_PETROSIAN BOOL FALSE 135 155 EXTENDED_SOURCE_ISOPHOTAL BOOL FALSE … … 155 175 156 176 # define the annuli (in pixels) for surface brightness measurements 157 @RADIAL.ANNULAR.BINS.LOWER F32 0.0 5.0 10.0 20.0 40.0 80.0 158 @RADIAL.ANNULAR.BINS.UPPER F32 5.0 10.0 20.0 40.0 80.0 160.0 177 # @RADIAL.ANNULAR.BINS.LOWER F32 0.0 5.0 10.0 20.0 40.0 80.0 178 # @RADIAL.ANNULAR.BINS.UPPER F32 5.0 10.0 20.0 40.0 80.0 160.0 179 180 # SDSS values: 181 @RADIAL.ANNULAR.BINS.LOWER F32 0.00 0.56 1.69 2.59 4.41 7.51 11.58 18.58 28.55 45.50 70.51 110.53 172.49 269.52 420.51 182 @RADIAL.ANNULAR.BINS.UPPER F32 0.56 1.69 2.59 4.41 7.51 11.58 18.58 28.55 45.50 70.51 110.53 172.49 269.52 420.51 652.50 159 183 160 184 # Extended source fit parameters … … 172 196 PETROSIAN_FLUX_RATIO F32 0.1 # we measure out to where flux = R0 * FLUX_RATIO 173 197 174 FITMODE STR BLEND175 DEBLEND_PEAK_FRACTION F32 0.1176 DEBLEND_SKY_NSIGMA F32 10.0177 178 198 # 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 part199 MEASURE.APTREND BOOL TRUE 180 200 APTREND STR CONSTANT 181 AP_MIN_SN F32 25.0201 AP_MIN_SN F32 0.0 # measure apMags for all sources by default 182 202 APTREND.NSTAR.MIN S32 5 183 203 APTREND.ORDER.MAX S32 5 … … 196 216 197 217 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?218 CONSTANT_PHOTOMETRIC_WEIGHTS BOOL FALSE 199 219 INTERPOLATE_AP BOOL TRUE 200 220 … … 207 227 NOISE.FACTOR F32 5.0 208 228 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 229 220 230 # alternate PSPHOT-type recipes … … 261 271 262 272 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 273 PSPHOT.EXT.NSIGMA.LIMIT F32 3.0 # sources with extNsigma greater that this get tagged as likely extended sources 274 PSPHOT.EXT.NSIGMA.MOMENTS F32 3.0 # sources with extNsigma greater that this get tagged as likely extended sources 264 275 PSPHOT.CR.GROW S32 1 # Number of pixels to grow CR mask 265 276 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights 266 277 PSPHOT.CRMASK.XTEST S32 0 278 PSPHOT.CRMASK.YTEST S32 0 279 PSPHOT.CRMASK.APPLY BOOL FALSE # TEST THIS before enabling. 280 281 # Detection efficiency 282 EFF.NUM S32 500 # Number of fake sources per bin 283 @EFF.MAG F32 -2.0 -1.0 -0.5 -0.25 -0.1 -0.05 0.0 0.05 0.1 0.25 0.5 1.0 2.0 # Magnitude of fake sources relative to limit 284 285 # stack photometry parameters 286 PSPHOT.STACK.MATCH.RADIUS F32 1.0 # join detections from different images with this correlation radius (pixels) 267 287 268 288 # Recipe overrides for CHIP … … 294 314 BACKGROUND.YBIN S32 2400 295 315 IMSTATS_NPIX S32 50000 296 END 316 BREAK_POINT STR ENSEMBLE 317 PEAKS_NMAX S32 1000 # on first pass, only keep NMAX peak (0 == all) 318 BACKGROUND.XBIN S32 128 # size of background superpixels 319 BACKGROUND.YBIN S32 128 # size of background superpixels 320 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background 321 END
Note:
See TracChangeset
for help on using the changeset viewer.
