Changeset 25756
- Timestamp:
- Oct 2, 2009, 3:13:59 PM (17 years ago)
- Location:
- trunk/ippconfig
- Files:
-
- 24 edited
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cfh12k/psphot.config (modified) (2 diffs)
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esowfi/psphot.config (modified) (1 diff)
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gpc1/psphot.config (modified) (2 diffs)
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isp/psphot.config (modified) (1 diff)
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lbc_red/psphot.config (modified) (1 diff)
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lulin/psphot.config (modified) (1 diff)
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megacam/psphot.config (modified) (1 diff)
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mosaic2/camera.config (modified) (1 diff)
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mosaic2/psphot.config (modified) (1 diff)
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recipes/ppSim.config (modified) (2 diffs)
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recipes/psphot.config (modified) (11 diffs)
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sdss/psphot.config (modified) (1 diff)
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sdssmosaic/psphot.config (modified) (3 diffs)
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simmosaic/psphot.config (modified) (1 diff)
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simple/psphot.config (modified) (1 diff)
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simtest/camera.config (modified) (1 diff)
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simtest/format.config (modified) (1 diff)
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simtest/ppSim.config (modified) (1 diff)
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simtest/psastro.config (modified) (3 diffs)
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simtest/psphot.config (modified) (1 diff)
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tek/psphot.config (modified) (1 diff)
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ucam/psphot.config (modified) (1 diff)
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uh8k/psphot.config (modified) (2 diffs)
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vysos5/psphot.config (modified) (1 diff)
Legend:
- Unmodified
- Added
- Removed
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trunk/ippconfig/cfh12k/psphot.config
r17291 r25756 1 1 2 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE4 SAVE.BACKMDL BOOL TRUE5 SAVE.PSF BOOL TRUE6 3 SAVE.PLOTS BOOL TRUE 7 8 BACKGROUND.XBIN S32 128 # size of background superpixels9 BACKGROUND.YBIN S32 128 # size of background superpixels10 11 # image background parameters12 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes:13 14 PSF_SN_LIM F32 50 # minimum S/N for stars used for PSF model15 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model16 17 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold18 PEAKS_NSIGMA_LIMIT_2 F32 10.0 # peak significance threshold19 4 20 5 # PSF model parameters : choose the PSF model desired 21 6 PSF_MODEL STR PS_MODEL_QGAUSS 22 7 23 MOMENTS_SN_MIN F32 20.0 # min S/N to measure moments 24 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 25 FULL_FIT_SN_LIM F32 50.0 26 AP_MIN_SN F32 25.0 27 MEASURE.APTREND BOOL FALSE 28 29 # BREAK_POINT may be one of (PEAKS, MOMENTS, PSFMODEL, ENSEMBLE) 30 # BREAK_POINT STR ENSEMBLE 31 32 OUTPUT.FORMAT STR PS1_DEV_1 33 34 # masking parameters (XXX EAM : rework this to use psRegion like ANALYSIS_REGION) 8 # XXX are these needed? 35 9 XMIN F32 +10 # minimum valid x-coord 36 10 XMAX F32 -10 # maximum valid x-coord … … 38 12 YMAX F32 -10 # maximum valid y-coord 39 13 40 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging -
trunk/ippconfig/esowfi/psphot.config
r15296 r25756 1 1 2 SAVE.BACKMDL BOOL TRUE 3 SAVE.BACKMDL.STDEV BOOL TRUE 4 SAVE.BACKGND BOOL TRUE 5 SAVE.BACKSUB BOOL TRUE 6 SAVE.PLOTS BOOL FALSE 7 SAVE.RESID BOOL TRUE 8 SAVE.PSF BOOL TRUE 9 LOAD.PSF BOOL FALSE 10 11 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes: 12 13 #PSPHOT_TEST METADATA 14 # SAVE.BACKSUB BOOL FALSE 15 # SAVE.RESID BOOL TRUE 16 #END 17 # 18 #PEAKS_OUTPUT_FILE STR peaks.dat 19 #MOMENTS_OUTPUT_FILE STR moments.dat 20 21 #PSF_SN_LIM F32 20.0 # minimum S/N for stars used for PSF model 22 MOMENTS_SN_MIN F32 20.0 # min S/N to measure moments 23 FULL_FIT_SN_LIM F32 100.0 24 EXT_MIN_SN F32 100.0 # fit galaxies above this S/N limit 25 26 PEAKS_NSIGMA_LIMIT F32 10.0 # peak significance threshold 27 BREAK_POINT STR ENSEMBLE # limit total processing for now (for speed) 28 29 30 SKY_STAT STR ROBUST_MEDIAN # statistic used to measure background 2 # choose the PSF model 3 PSF_MODEL STR PS_MODEL_QGAUSS -
trunk/ippconfig/gpc1/psphot.config
r24402 r25756 1 1 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE 4 SAVE.BACKMDL BOOL TRUE 5 SAVE.PSF BOOL TRUE 6 SAVE.PLOTS BOOL TRUE 2 BACKGROUND.XBIN S32 256 # size of background superpixels 3 BACKGROUND.YBIN S32 256 # size of background superpixels 7 4 8 # for testing: 9 # BREAK_POINT STR BACKMDL 5 SOFTEN.VARIANCE BOOL TRUE # XXX drop? soften the errors for bright pixels 6 SOFTEN.VARIANCE.FRACTION F32 0.005 10 7 11 BACKGROUND.XBIN S32 256 # size of background superpixels 12 BACKGROUND.YBIN S32 256 # size of background superpixels 8 PEAKS_SMOOTH_SIGMA F32 2.5 # smoothing kernel sigma in pixels 13 9 14 # image background parameters 15 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 16 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background 17 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background 10 PSF_CLUMP_NX S32 3 # subdivide image in to NX x NY regions for 11 PSF_CLUMP_NY S32 3 # selecting PSF stars 12 PSF_CLUMP_GRID_SCALE F32 2.5 # XXX too large? size of Sx,Sy image pixel 18 13 19 PEAKS_SMOOTH_SIGMA F32 2.5 # smoothing kernel sigma in pixels 20 PEAKS_NMAX S32 5000 # on first pass, only keep NMAX peaks (0 == all) 21 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold 22 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold 23 24 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model 25 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 26 PSF_CLUMP_NX S32 3 # subdivide image in to NX x NY regions for 27 PSF_CLUMP_NY S32 3 # selecting PSF stars 28 PSF_MOMENTS_RADIUS F32 12 # calculate initial source moments with this radius 29 PSF_CLUMP_GRID_SCALE F32 2.5 # size of Sx,Sy image pixel 30 31 PSF.RESIDUALS BOOL TRUE # generate the residuals? 14 PSF.RESIDUALS.RADIUS F32 9.0 # keep this pixel if residual is more significant than this 15 PSF.RESIDUALS.SPATIAL_ORDER S32 1 # fit spatial variations of the residuals at this order (0,1) 32 16 33 17 # PSF model parameters : choose the PSF model desired 34 PSF_MODEL STRPS_MODEL_PS1_V135 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights18 PSF_MODEL STR PS_MODEL_PS1_V1 19 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights in CR stat 36 20 37 PSF.TREND.MODE STR MAP # other options: POLY_CHEB, POLY_ORD38 21 PSF.TREND.NX S32 3 39 22 PSF.TREND.NY S32 3 40 23 41 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 42 FULL_FIT_SN_LIM F32 25.0 43 MOMENTS_SN_MIN F32 5.0 44 AP_MIN_SN F32 5.0 24 # rename NONLINEAR_FIT_SN_LIM? 25 FULL_FIT_SN_LIM F32 25.0 45 26 46 OUTPUT.FORMAT STR PS1_V2 27 APTREND.ORDER.MAX S32 3 47 28 48 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation 49 PSF_MAX_CHI F32 50.0 # reject objects worse that this 50 51 MEASURE.APTREND BOOL TRUE ### XXX for now, skip this (too many errors) 52 APTREND.ORDER.MAX S32 3 53 54 DIAGNOSTIC.PLOTS METADATA 29 DIAGNOSTIC.PLOTS METADATA 55 30 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE 56 31 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 32 … … 58 33 END 59 34 60 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 61 62 DIFF METADATA 63 BACKGROUND.XBIN S32 32 # size of background superpixels 64 BACKGROUND.YBIN S32 32 # size of background superpixels 35 DIFF METADATA 36 BACKGROUND.XBIN S32 32 # size of background superpixels 37 BACKGROUND.YBIN S32 32 # size of background superpixels 65 38 END -
trunk/ippconfig/isp/psphot.config
r15044 r25756 1 1 2 2 # turn these on to see specific outputs 3 SAVE.BACKMDL BOOL TRUE4 SAVE.BACKGND BOOL TRUE5 SAVE.BACKSUB BOOL TRUE6 SAVE.RESID BOOL TRUE7 SAVE.PSF BOOL TRUE8 3 SAVE.PLOTS BOOL TRUE 9 4 10 # image statistics parameters 11 IMSTATS_NPIX S32 5000 # number of pixels to use for sky estimate boxes: 12 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background 13 14 PSF_SN_LIM F32 30 # minimum S/N for stars used for PSF model 15 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 16 5 # PSF model parameters : choose the PSF model 17 6 PSF_MODEL STR PS_MODEL_PGAUSS 18 7 19 MOMENTS_SN_MIN F32 30.0 20 MOMENTS_AR_MAX F32 2.0 # maximum axial ratio: 1 / AR < (sx / sy) < AR 21 22 #EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 23 #FULL_FIT_SN_LIM F32 50.0 24 #AP_MIN_SN F32 20.0 8 # xxx check this: 25 9 PSF_CLUMP_NSIGMA F32 3.5 # region of Sx,Sy plane to use for selecting PSF stars 26 10 27 # PSFTREND must be a 2D polynomial 28 # the specified values are ignored but define the active components of the polynomial 29 PSF.TREND.MASK METADATA 30 NORDER_X S32 3 # number of x orders 31 NORDER_Y S32 3 # number of y orders 32 VAL_X00_Y00 F64 1 # polynomial coefficient 33 34 VAL_X01_Y00 F64 1 # polynomial coefficient 35 VAL_X00_Y01 F64 1 # polynomial coefficient 36 37 VAL_X02_Y00 F64 1 # polynomial coefficient 38 VAL_X01_Y01 F64 1 # polynomial coefficient 39 VAL_X00_Y02 F64 1 # polynomial coefficient 40 41 VAL_X03_Y00 F64 1 # polynomial coefficient 42 VAL_X02_Y01 F64 1 # polynomial coefficient 43 VAL_X01_Y02 F64 1 # polynomial coefficient 44 VAL_X00_Y03 F64 1 # polynomial coefficient 45 NELEMENTS S32 10 # number of unmasked components 46 END # folder for 4D polynomial 47 11 # XXX set other 2D trends 48 12 PSF.TREND.NX S32 4 49 13 PSF.TREND.NY S32 4 50 51 XMIN F32 1552 53 PSF.RESIDUALS BOOL true54 PSF.RESIDUALS.SPATIAL_ORDER S32 155 56 BREAK_POINT STR ENSEMBLE57 OUTPUT.FORMAT STR PS1_DEV_058 59 PSPHOT.SUMMIT METADATA60 PEAKS_SMOOTH_SIGMA F32 0.8 # peak significance threshold61 PEAKS_NSIGMA_LIMIT F32 50.0 # peak significance threshold62 PEAKS_NMAX S32 100063 SAVE.RESID BOOL FALSE64 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model65 MOMENTS_SN_MIN F32 25.066 PSF_MODEL STR PS_MODEL_PGAUSS67 END68 69 DIAGNOSTIC.PLOTS METADATA70 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE71 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 472 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 773 END74 75 SKY_BIAS F32 0.576 AP_MIN_SN F32 30.0 -
trunk/ippconfig/lbc_red/psphot.config
r17154 r25756 1 1 2 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE4 SAVE.BACKMDL BOOL TRUE5 SAVE.PSF BOOL TRUE6 3 SAVE.PLOTS BOOL TRUE 7 8 BACKGROUND.XBIN S32 128 # size of background superpixels9 BACKGROUND.YBIN S32 128 # size of background superpixels10 11 # image background parameters12 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes:13 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background14 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background15 16 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model17 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model18 4 19 5 # PSF model parameters : choose the PSF model desired 20 6 PSF_MODEL STR PS_MODEL_QGAUSS 21 22 MOMENTS_SN_MIN F32 30.023 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit24 FULL_FIT_SN_LIM F32 50.025 AP_MIN_SN F32 50.026 27 # OUTPUT.FORMAT STR SMPDATA28 OUTPUT.FORMAT STR PS1_DEV_129 30 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation31 PSF_MAX_CHI F32 50.0 # reject objects worse that this32 33 #PSF.TREND.MODE STR MAP34 #PSF.TREND.NX S32 135 #PSF.TREND.NY S32 136 37 DIAGNOSTIC.PLOTS METADATA38 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE39 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 -140 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 1241 END42 -
trunk/ippconfig/lulin/psphot.config
r18436 r25756 1 1 2 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE4 SAVE.BACKMDL BOOL TRUE5 SAVE.PSF BOOL TRUE6 3 SAVE.PLOTS BOOL TRUE 7 8 BACKGROUND.XBIN S32 128 # size of background superpixels9 BACKGROUND.YBIN S32 128 # size of background superpixels10 11 # image background parameters12 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes:13 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background14 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background15 16 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model17 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model18 4 19 5 # PSF model parameters : choose the PSF model desired 20 6 PSF_MODEL STR PS_MODEL_QGAUSS 21 22 MOMENTS_SN_MIN F32 30.023 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit24 FULL_FIT_SN_LIM F32 50.025 AP_MIN_SN F32 50.026 27 # OUTPUT.FORMAT STR SMPDATA28 OUTPUT.FORMAT STR PS1_DEV_129 30 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation31 PSF_MAX_CHI F32 50.0 # reject objects worse that this32 33 #PSF.TREND.MODE STR MAP34 #PSF.TREND.NX S32 135 #PSF.TREND.NY S32 136 37 DIAGNOSTIC.PLOTS METADATA38 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE39 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 -140 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 1241 END42 43 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging -
trunk/ippconfig/megacam/psphot.config
r24893 r25756 1 1 2 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE4 SAVE.BACKMDL BOOL TRUE5 SAVE.PSF BOOL TRUE6 3 SAVE.PLOTS BOOL TRUE 7 8 BACKGROUND.XBIN S32 128 # size of background superpixels9 BACKGROUND.YBIN S32 128 # size of background superpixels10 11 # image background parameters12 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes:13 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background14 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background15 16 PSF_SN_LIM F32 20 # minimum S/N for stars used for PSF model17 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model18 4 19 5 # PSF model parameters : choose the PSF model desired 20 6 PSF_MODEL STR PS_MODEL_QGAUSS 21 7 22 PSF_MOMENTS_RADIUS F32 10.0 # calculate initial source moments with this radius23 24 MOMENTS_SN_MIN F32 2.025 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit26 FULL_FIT_SN_LIM F32 10.027 AP_MIN_SN F32 2.028 29 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation30 PSF_MAX_CHI F32 50.0 # reject objects worse that this31 32 8 PSF.TREND.MODE STR MAP 33 9 PSF.TREND.NX S32 1 34 10 PSF.TREND.NY S32 1 35 36 DIAGNOSTIC.PLOTS METADATA37 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE38 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 -139 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 1240 END41 42 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging43 44 PEAKS_NSIGMA_LIMIT F32 10.0 -
trunk/ippconfig/mosaic2/camera.config
r19019 r25756 90 90 CMF.XSRC STR {CHIP.NAME}.xsrc # use .PSF and .EXT? 91 91 CMF.XFIT STR {CHIP.NAME}.xfit # use .PSF and .EXT? 92 CMF.DETEFF STR {CHIP.NAME}.deteff 92 93 93 94 PSF.HEAD STR {CHIP.NAME}.hdr -
trunk/ippconfig/mosaic2/psphot.config
r19864 r25756 1 1 2 # turn these on to see specific outputs 3 SAVE.RESID BOOL TRUE 2 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 4 3 5 IMSTATS_NPIX S32 1000 # number of pixels to use for sky estimate boxes: 4 # robust vs fitted?? gpc1 uses fitted... robust median gives better background stdev --> test with flat-field photometry 5 SKY_STAT STR ROBUST_MEDIAN # statistic used to measure background 6 6 7 PSF_ SN_LIM F32 20 # minimum S/N for stars used for PSF model8 PSF_MAX_NSTARS S32 300# limit number of stars used for PSF model7 PSF_MODEL STR PS_MODEL_QGAUSS 8 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 9 9 10 # PSF model parameters : choose the PSF model 11 # list as many PSF_MODEL options as desired 12 # if you want to list multiple entries, uncomment 'MULTI' here 13 # PSF_MODEL MULTI 14 PSF_MODEL STR PS_MODEL_QGAUSS 15 # PSF_MODEL STR PS_MODEL_GAUSS 16 # PSF_MODEL STR PS_MODEL_PGAUSS 17 # PSF_MODEL STR PS_MODEL_TGAUSS ## not well tested, not very successful 10 # Mosaic 2 has substantial IQ variations in the y-direction 11 PSF_CLUMP_NX S32 1 # subdivide image in to NX x NY regions for 12 PSF_CLUMP_NY S32 3 # selecting PSF stars 18 13 19 MOMENTS_SN_MIN F32 10.0 # min S/N to measure moments 20 EXT_MIN_SN F32 20.0 # fit galaxies above this S/N limit 21 FULL_FIT_SN_LIM F32 20.0 22 AP_MIN_SN F32 25.0 14 # Mosaic 2 has substantial IQ variations in the y-direction 15 PSF.TREND.NX S32 1 16 PSF.TREND.NY S32 3 23 17 24 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 18 PEAKS_NSIGMA_LIMIT F32 15.0 # peak significance threshold 19 FOOTPRINT_NSIGMA_LIMIT F32 14.0 # threshold for bright pmFootprint detection 25 20 26 ## gene's overrides for testing: 27 PEAKS_NSIGMA_LIMIT_2 F32 10.0 # peak significance threshold 21 PSF_SN_LIM F32 20.0 # minimum S/N for stars used for PSF model 22 FULL_FIT_SN_LIM F32 10.0 23 EXT_MIN_SN F32 10.0 # fit galaxies above this S/N limit 28 24 29 EXT_MODEL STRPS_MODEL_QGAUSS25 EXT_MODEL STR PS_MODEL_QGAUSS 30 26 31 TEST_FIT BOOL FALSE 32 TEST_FIT_X F32 781 33 TEST_FIT_Y F32 830 27 EXTENDED_SOURCE_SN_LIM F32 3.0 28 #EXTENDED_SOURCE_ANALYSIS BOOL TRUE # perform any of the aperture-like measurements? 29 #EXTENDED_SOURCE_PETROSIAN BOOL TRUE 34 30 35 TEST_FIT_MODE STR CONV 36 #TEST_FIT_MODE STR PSF 37 #TEST_FIT_MODE STR EXT 38 39 #TEST_FIT_MODEL STR PS_MODEL_SERSIC 40 TEST_FIT_MODEL STR PS_MODEL_QGAUSS 41 TEST_MOMENTS_RADIUS F32 9.0 42 OUTPUT.FORMAT STR PS1_DEV_1 43 44 PSF_MOMENTS_RADIUS F32 7 # calculate initial source moments with this radius 31 # 3 to match PSF and Moments 2D variations 32 APTREND.ORDER.MAX S32 3 -
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 -
trunk/ippconfig/sdss/psphot.config
r14644 r25756 1 2 # turn these on to see specific outputs3 SAVE.BACKMDL BOOL TRUE4 #SAVE.BACKGND BOOL TRUE5 #SAVE.BACKSUB BOOL TRUE6 #SAVE.RESID BOOL TRUE7 SAVE.PSF BOOL TRUE8 SAVE.PLOTS BOOL TRUE9 10 # image statistics parameters11 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes:12 13 PSF_SN_LIM F32 10 # minimum S/N for stars used for PSF model14 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model15 1 16 2 PSF_MODEL STR PS_MODEL_QGAUSS 17 3 18 MOMENTS_SN_MIN F32 10.0 19 #EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 20 #FULL_FIT_SN_LIM F32 50.0 21 #AP_MIN_SN F32 20.0 4 # check: 22 5 PSF_CLUMP_NSIGMA F32 2.5 # region of Sx,Sy plane to use for selecting PSF stars 23 6 24 # PSFTREND must be a 2D polynomial 25 # the specified values are ignored but define the active components of the polynomial 26 PSF.TREND.MASK METADATA 27 NORDER_X S32 3 # number of x orders 28 NORDER_Y S32 3 # number of y orders 29 VAL_X00_Y00 F64 1 # polynomial coefficient 30 31 VAL_X01_Y00 F64 1 # polynomial coefficient 32 VAL_X00_Y01 F64 1 # polynomial coefficient 33 34 VAL_X02_Y00 F64 1 # polynomial coefficient 35 VAL_X01_Y01 F64 1 # polynomial coefficient 36 VAL_X00_Y02 F64 1 # polynomial coefficient 37 38 VAL_X03_Y00 F64 1 # polynomial coefficient 39 VAL_X02_Y01 F64 1 # polynomial coefficient 40 VAL_X01_Y02 F64 1 # polynomial coefficient 41 VAL_X00_Y03 F64 1 # polynomial coefficient 42 NELEMENTS S32 10 # number of unmasked components 43 END # folder for 4D polynomial 44 7 # is this needed to mask bad regions? 45 8 XMIN F32 15 46 47 PSF.RESIDUALS BOOL true48 PSF.RESIDUALS.SPATIAL_ORDER S32 149 50 # BREAK_POINT STR ENSEMBLE51 OUTPUT.FORMAT STR PS1_DEV_052 53 PSPHOT.SUMMIT METADATA54 PEAKS_SMOOTH_SIGMA F32 0.8 # peak significance threshold55 PEAKS_NSIGMA_LIMIT F32 50.0 # peak significance threshold56 PEAKS_NMAX S32 100057 SAVE.RESID BOOL FALSE58 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model59 MOMENTS_SN_MIN F32 25.060 PSF_MODEL STR PS_MODEL_PGAUSS61 END -
trunk/ippconfig/sdssmosaic/psphot.config
r24067 r25756 1 2 # turn these on to see specific outputs3 SAVE.OUTPUT BOOL TRUE4 SAVE.BACKMDL BOOL TRUE5 #SAVE.RESID BOOL TRUE6 #SAVE.BACKGND BOOL TRUE7 SAVE.BACKSUB BOOL TRUE8 SAVE.PSF BOOL TRUE9 #LOAD.PSF BOOL FALSE10 #SAVE.PLOTS BOOL TRUE11 12 # for testing:13 # BREAK_POINT STR BACKMDL14 15 1 16 2 BACKGROUND.XBIN S32 256 # size of background superpixels 17 3 BACKGROUND.YBIN S32 256 # size of background superpixels 18 4 19 # image background parameters 20 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 21 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background 22 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background 23 24 PEAKS_SMOOTH_SIGMA F32 2.5 # smoothing kernel sigma in pixels 25 PEAKS_NMAX S32 5000 # on first pass, only keep NMAX peaks (0 == all) 26 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold 27 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold 28 29 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model 30 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 5 # what is the 2D variation of the SDSS PSF? 31 6 PSF_CLUMP_NX S32 3 # subdivide image in to NX x NY regions for 32 7 PSF_CLUMP_NY S32 3 # selecting PSF stars 33 PSF_MOMENTS_RADIUS F32 12 # calculate initial source moments with this radius 8 9 # test this: 34 10 PSF_CLUMP_GRID_SCALE F32 2.5 # size of Sx,Sy image pixel 35 36 PSF.RESIDUALS BOOL TRUE # generate the residuals?37 11 38 12 # PSF model parameters : choose the PSF model desired 39 13 PSF_MODEL STR PS_MODEL_PS1_V1 40 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights41 14 42 15 # Use same default setting as in 2.6.1 (MAP is now global default) … … 45 18 PSF.TREND.NY S32 0 46 19 47 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 48 FULL_FIT_SN_LIM F32 25.0 49 MOMENTS_SN_MIN F32 5.0 50 AP_MIN_SN F32 5.0 51 52 OUTPUT.FORMAT STR PS1_V1 53 54 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation 55 PSF_MAX_CHI F32 50.0 # reject objects worse that this 56 57 MEASURE.APTREND BOOL TRUE ### XXX for now, skip this (too many errors) 58 APTREND.ORDER.MAX S32 3 59 60 # BREAK_POINT STR PASS1 61 20 # match the SDSS radius: 62 21 PSF_REF_RADIUS F32 18.7 # aperture magnitudes are scaled via 63 22 # curve-of-growth to this radius 64 65 DIAGNOSTIC.PLOTS METADATA 66 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE 67 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 32 68 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 15 69 END 70 71 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 72 73 # Default is noap, nopsf; following recipes turn on one or both of these 74 23 # for tests: Default is noap, nopsf; following recipes turn on one or both of these 75 24 PSPHOT_NOAP_PSF METADATA 76 25 PSF.TREND.MODE STR MAP … … 96 45 END 97 46 47 # put these values in the master? 98 48 DIFF METADATA 99 49 BACKGROUND.XBIN S32 32 # size of background superpixels -
trunk/ippconfig/simmosaic/psphot.config
r20889 r25756 1 1 2 SAVE.BACKMDL BOOL TRUE 3 SAVE.BACKGND BOOL TRUE 4 SAVE.BACKSUB BOOL TRUE 5 SAVE.PLOTS BOOL FALSE 6 SAVE.RESID BOOL TRUE 7 SAVE.PSF BOOL TRUE 8 LOAD.PSF BOOL FALSE 9 10 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes: 11 SKY_INNER_RADIUS F32 10 # square annulus for local sky measurement 12 13 PSF_MOMENTS_RADIUS F32 7 # calculate initial source moments with this radius 14 15 16 17 #PSPHOT_TEST METADATA 18 # SAVE.BACKSUB BOOL FALSE 19 # SAVE.RESID BOOL TRUE 20 #END 21 # 22 #PEAKS_OUTPUT_FILE STR peaks.dat 23 #MOMENTS_OUTPUT_FILE STR moments.dat 24 25 #PSF_SN_LIM F32 20.0 # minimum S/N for stars used for PSF model 26 MOMENTS_SN_MIN F32 10.0 # min S/N to measure moments 27 FULL_FIT_SN_LIM F32 100.0 28 EXT_MIN_SN F32 100.0 # fit galaxies above this S/N limit 29 30 MOMENTS_SX_MAX F32 25.0 31 MOMENTS_SY_MAX F32 25.0 32 33 34 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold 35 PEAKS_NSIGMA_LIMIT_2 F32 10.0 # peak significance threshold 36 37 BREAK_POINT STR ENSEMBLE # limit total processing for now (for speed) 38 39 40 SKY_STAT STR ROBUST_MEDIAN # statistic used to measure background 2 # ppSim currently uses PS_MODEL_GAUSS 3 PSF_MODEL STR PS_MODEL_PGAUSS -
trunk/ippconfig/simple/psphot.config
r19320 r25756 1 1 2 SAVE.BACKMDL BOOL FALSE3 SAVE.BACKGND BOOL FALSE4 SAVE.BACKSUB BOOL FALSE5 SAVE.PLOTS BOOL TRUE6 2 SAVE.RESID BOOL TRUE 7 SAVE.PSF BOOL TRUE8 LOAD.PSF BOOL FALSE9 10 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes:11 12 MOMENTS_SN_MIN F32 20.0 # min S/N to measure moments13 FULL_FIT_SN_LIM F32 100.014 EXT_MIN_SN F32 100.0 # fit galaxies above this S/N limit15 16 PEAKS_NSIGMA_LIMIT F32 10.0 # peak significance threshold17 USE_FOOTPRINTS BOOL T # use new pmFootprint peak packaging -
trunk/ippconfig/simtest/camera.config
r24808 r25756 64 64 CMF.XSRC STR {CHIP.NAME}.xsrc # use .PSF and .EXT? 65 65 CMF.XFIT STR {CHIP.NAME}.xfit # use .PSF and .EXT? 66 CMF.DETEFF STR {CHIP.NAME}.deteff 66 67 67 68 PSF.HEAD STR {CHIP.NAME}.hdr -
trunk/ippconfig/simtest/format.config
r24808 r25756 69 69 CELL.X0 S32 0 70 70 CELL.Y0 S32 0 71 CELL.XSIZE S32 204872 CELL.YSIZE S32 204871 CELL.XSIZE S32 1024 72 CELL.YSIZE S32 1024 73 73 CELL.XWINDOW S32 0 74 74 CELL.YWINDOW S32 0 -
trunk/ippconfig/simtest/ppSim.config
r25728 r25756 9 9 BIAS BOOL FALSE 10 10 FLAT BOOL FALSE 11 BIAS.LEVEL F32 1000.0 # Bias level (e) 12 BIAS.RANGE F32 20.0 # Range of bias values (e) 13 BIAS.ORDER S32 7 # Order for overscan polynomial 14 15 STARS.MAG F32 10.0 # Brightest magnitude for fake stars 16 STARS.DENSITY F32 100.0 # Stellar density (per square degree) at the brightest magnitude 17 STARS.SIGMA.LIM F32 5.0 # significance of faintest sources 18 STARS.LUM F32 0.35 # Stellar luminosity function slope (magnitude slope) 19 END 20 21 # for a quick test, we are going to skip shutter and dark corrections 22 STACKTEST.MAKE METADATA 23 PSF.MODEL STR PS_MODEL_PGAUSS 24 SHUTTER.TIME F32 0.0 25 DARK.RATE F32 0.0 26 SCATTER.FRAC F32 0.0 27 BIAS BOOL FALSE 28 FLAT BOOL FALSE 11 29 BIAS.LEVEL F32 1000.0 # Bias level (e) 12 30 BIAS.RANGE F32 20.0 # Range of bias values (e) 13 31 BIAS.ORDER S32 7 # Order for overscan polynomial 32 33 # generate a set of fake stars 34 STARS.REAL BOOL FALSE # Add stars from a catalogue? 35 STARS.FAKE BOOL TRUE # Add fake stars, randomly distributed? 36 MATCH.DENSITY BOOL TRUE # significance of faintest sources 37 38 EXPTIME F32 10.0 39 RA F32 5.0 40 DEC F32 5.0 41 PA F32 0.0 42 SEEING F32 1.0 43 SCALE F32 0.25 44 ZEROPOINT F32 25.0 45 SKY.MAGS F32 22.0 14 46 END 15 47 48 # for a quick test, we are going to skip shutter and dark corrections 49 STACKTEST.RUN METADATA 50 PSF.MODEL STR PS_MODEL_GAUSS 51 SHUTTER.TIME F32 0.0 52 DARK.RATE F32 0.0 53 SCATTER.FRAC F32 0.0 54 BIAS BOOL FALSE 55 FLAT BOOL FALSE 56 BIAS.LEVEL F32 1000.0 # Bias level (e) 57 BIAS.RANGE F32 20.0 # Range of bias values (e) 58 BIAS.ORDER S32 7 # Order for overscan polynomial 59 60 # generate a set of fake stars 61 STARS.REAL BOOL TRUE # Add stars from a catalogue? 62 STARS.FAKE BOOL FALSE # Add fake stars, randomly distributed? 63 MATCH.DENSITY BOOL TRUE # significance of faintest sources 64 65 EXPTIME F32 10.0 66 RA F32 5.0 67 DEC F32 5.0 68 PA F32 0.0 69 SEEING F32 1.0 70 SCALE F32 0.25 71 ZEROPOINT F32 25.0 72 SKY.MAGS F32 22.0 73 END 74 -
trunk/ippconfig/simtest/psastro.config
r24032 r25756 3 3 4 4 PSASTRO.GRID.OFFSET F32 500. 5 PSASTRO.GRID.SCALE F32 50.5 PSASTRO.GRID.SCALE F32 10. 6 6 7 7 PSASTRO.IGNORE STR CRLIMIT,SATURATED,DEFECT,BLEND … … 9 9 PSASTRO.CATDIR STR SYNTH.SIMTEST 10 10 DVO.GETSTAR.PHOTCODE STR r 11 PSASTRO.MAX.NSTAR S32 50 # max stars accepted for fitting11 PSASTRO.MAX.NSTAR S32 200 # max stars accepted for fitting 12 12 DVO.GETSTAR.MAX.RHO F32 10000.0 13 13 DVO.GETSTAR.MIN.MAG F32 10.0 … … 34 34 PHOTCODE STR z_SYNTH 35 35 END 36 -
trunk/ippconfig/simtest/psphot.config
r19947 r25756 1 1 2 SAVE.BACKMDL BOOL TRUE 3 SAVE.BACKGND BOOL TRUE 4 SAVE.BACKSUB BOOL TRUE 5 SAVE.PLOTS BOOL TRUE 6 SAVE.RESID BOOL TRUE 7 SAVE.PSF BOOL TRUE 8 LOAD.PSF BOOL FALSE 9 10 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes: 11 SKY_INNER_RADIUS F32 10 # square annulus for local sky measurement 12 13 PSF_MOMENTS_RADIUS F32 7 # calculate initial source moments with this radius 14 15 #PSPHOT_TEST METADATA 16 # SAVE.BACKSUB BOOL FALSE 17 # SAVE.RESID BOOL TRUE 18 #END 19 # 20 #PEAKS_OUTPUT_FILE STR peaks.dat 21 #MOMENTS_OUTPUT_FILE STR moments.dat 22 23 #PSF_SN_LIM F32 20.0 # minimum S/N for stars used for PSF model 24 MOMENTS_SN_MIN F32 10.0 # min S/N to measure moments 25 FULL_FIT_SN_LIM F32 100.0 26 EXT_MIN_SN F32 100.0 # fit galaxies above this S/N limit 27 28 MOMENTS_SX_MAX F32 25.0 29 MOMENTS_SY_MAX F32 25.0 30 31 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold 32 PEAKS_NSIGMA_LIMIT_2 F32 10.0 # peak significance threshold 33 BREAK_POINT STR NONE # limit total processing for now (for speed) 34 35 36 SKY_STAT STR ROBUST_MEDIAN # statistic used to measure background 2 # same as ppSim.config (if YES, <apResid> should be 0.0) 3 # ppSim currently uses PS_MODEL_GAUSS 4 PSF_MODEL STR PS_MODEL_PGAUSS -
trunk/ippconfig/tek/psphot.config
r14564 r25756 1 2 # turn these on to see specific outputs3 #SAVE.BACKMDL BOOL TRUE4 #SAVE.BACKGND BOOL TRUE5 #SAVE.BACKSUB BOOL TRUE6 SAVE.RESID BOOL TRUE7 #SAVE.PSF BOOL TRUE8 9 # image statistics parameters10 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes:11 12 PSF_SN_LIM F32 10 # minimum S/N for stars used for PSF model13 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model14 1 15 2 PSF_MODEL STR PS_MODEL_QGAUSS 16 3 17 MOMENTS_SN_MIN F32 10.018 #EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit19 #FULL_FIT_SN_LIM F32 50.020 #AP_MIN_SN F32 20.021 PSF_CLUMP_NSIGMA F32 2.5 # region of Sx,Sy plane to use for selecting PSF stars22 23 # PSFTREND must be a 2D polynomial24 # the specified values are ignored but define the active components of the polynomial25 PSF.TREND.MASK METADATA26 NORDER_X S32 3 # number of x orders27 NORDER_Y S32 3 # number of y orders28 VAL_X00_Y00 F64 1 # polynomial coefficient29 30 VAL_X01_Y00 F64 1 # polynomial coefficient31 VAL_X00_Y01 F64 1 # polynomial coefficient32 33 VAL_X02_Y00 F64 1 # polynomial coefficient34 VAL_X01_Y01 F64 1 # polynomial coefficient35 VAL_X00_Y02 F64 1 # polynomial coefficient36 37 VAL_X03_Y00 F64 1 # polynomial coefficient38 VAL_X02_Y01 F64 1 # polynomial coefficient39 VAL_X01_Y02 F64 1 # polynomial coefficient40 VAL_X00_Y03 F64 1 # polynomial coefficient41 NELEMENTS S32 10 # number of unmasked components42 END # folder for 4D polynomial43 44 XMIN F32 1545 PSF.RESIDUALS BOOL false46 BREAK_POINT STR ENSEMBLE47 OUTPUT.FORMAT STR PS1_DEV_048 49 PSPHOT.SUMMIT METADATA50 PEAKS_SMOOTH_SIGMA F32 0.8 # peak significance threshold51 PEAKS_NSIGMA_LIMIT F32 50.0 # peak significance threshold52 PEAKS_NMAX S32 100053 SAVE.RESID BOOL FALSE54 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model55 MOMENTS_SN_MIN F32 25.056 PSF_MODEL STR PS_MODEL_PGAUSS57 END -
trunk/ippconfig/ucam/psphot.config
r12376 r25756 1 1 2 # turn these on to see specific outputs3 #SAVE.BACKMDL BOOL TRUE4 #SAVE.BACKGND BOOL TRUE5 #SAVE.BACKSUB BOOL TRUE6 SAVE.RESID BOOL TRUE7 #SAVE.PSF BOOL TRUE8 #LOAD.PSF BOOL FALSE9 10 IMSTATS_NPIX S32 1000 # number of pixels to use for sky estimate boxes:11 12 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model13 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model14 15 # PSF model parameters : choose the PSF model16 # list as many PSF_MODEL options as desired17 # if you want to list multiple entries, uncomment 'MULTI' here18 # PSF_MODEL MULTI19 2 PSF_MODEL STR PS_MODEL_QGAUSS 20 # PSF_MODEL STR PS_MODEL_GAUSS21 # PSF_MODEL STR PS_MODEL_PGAUSS22 # PSF_MODEL STR PS_MODEL_TGAUSS ## not well tested, not very successful23 24 MOMENTS_SN_MIN F32 20.0 # min S/N to measure moments25 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit26 FULL_FIT_SN_LIM F32 50.027 AP_MIN_SN F32 25.0 -
trunk/ippconfig/uh8k/psphot.config
r18442 r25756 1 2 # turn these on to see specific outputs3 SAVE.OUTPUT BOOL TRUE4 SAVE.BACKMDL BOOL TRUE5 SAVE.PSF BOOL TRUE6 SAVE.PLOTS BOOL TRUE7 8 BACKGROUND.XBIN S32 128 # size of background superpixels9 BACKGROUND.YBIN S32 128 # size of background superpixels10 11 # image background parameters12 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes:13 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background14 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background15 16 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model17 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model18 1 19 2 # PSF model parameters : choose the PSF model desired 20 3 PSF_MODEL STR PS_MODEL_QGAUSS 21 22 MOMENTS_SN_MIN F32 30.023 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit24 FULL_FIT_SN_LIM F32 50.025 AP_MIN_SN F32 50.026 27 # OUTPUT.FORMAT STR SMPDATA28 OUTPUT.FORMAT STR PS1_DEV_129 30 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation31 PSF_MAX_CHI F32 50.0 # reject objects worse that this32 33 #PSF.TREND.MODE STR MAP34 #PSF.TREND.NX S32 135 #PSF.TREND.NY S32 136 4 37 5 DIAGNOSTIC.PLOTS METADATA … … 40 8 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 12 41 9 END 42 43 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging -
trunk/ippconfig/vysos5/psphot.config
r20652 r25756 1 1 2 SAVE.BACKMDL BOOL TRUE 3 SAVE.BACKGND BOOL FALSE 4 SAVE.BACKSUB BOOL FALSE 5 SAVE.PLOTS BOOL TRUE 6 SAVE.RESID BOOL FALSE 7 SAVE.PSF BOOL TRUE 8 LOAD.PSF BOOL FALSE 2 # XXX check on this value 3 PSF_CLUMP_NSIGMA F32 3.5 # region of Sx,Sy plane to use for selecting PSF stars 9 4 10 PEAKS_NSIGMA_LIMIT F32 20.0 # peak significance threshold 11 PEAKS_NSIGMA_LIMIT_2 F32 10.0 # peak significance threshold 12 PSF_MOMENTS_RADIUS F32 7 # calculate initial source moments with this radius 13 PSF_CLUMP_NSIGMA F32 3.5 # region of Sx,Sy plane to use for selecting PSF stars 14 PSF_MAX_NSTARS S32 400 # limit number of stars used for PSF model 15 MEASURE.APTREND BOOL TRUE 16 5 # do we want to do 2-pass analysis? 17 6 BREAK_POINT STR PASS1 18 7 8 # keep these large since psfs are so undersampled 19 9 PSPHOT.CR.NSIGMA.LIMIT F32 5.0 # sources with crNsigma greater that this get tagged as likely cosmic rays 20 10 PSPHOT.EXT.NSIGMA.LIMIT F32 5.0 # sources with extNsigma greater that this get tagged as likely extended sources 21 11 22 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 23 FOOTPRINT_NPIXMIN S32 5 # Minimum size of a pmFootprint 24 FOOTPRINT_NSIGMA_LIMIT F32 10 # threshold for bright pmFootprint detection 25 FOOTPRINT_NSIGMA_LIMIT_2 F32 10 # threshold for faint pmFootprint detection 12 # small psfs so small grow radius 26 13 FOOTPRINT_GROW_RADIUS S32 1 # How much to grow bright footprints 27 14 FOOTPRINT_GROW_RADIUS_2 S32 2 # How much to grow faint footprints 28 FOOTPRINT_CULL_NSIGMA_DELTA F32 4 # Cull peaks that aren't nsigma above coll to neighbour29 FOOTPRINT_CULL_NSIGMA_MIN F32 1 # Minimum height of colls in units of skyStdev30 15 31 16 PSF_MODEL STR PS_MODEL_PGAUSS
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