Changeset 25727
- Timestamp:
- Oct 1, 2009, 2:07:04 PM (17 years ago)
- Location:
- branches/eam_branches/20090715/ippconfig
- Files:
-
- 16 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) (4 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/psphot.config (modified) (1 diff)
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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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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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branches/eam_branches/20090715/ippconfig/cfh12k/psphot.config
r17291 r25727 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 -
branches/eam_branches/20090715/ippconfig/esowfi/psphot.config
r15296 r25727 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 -
branches/eam_branches/20090715/ippconfig/gpc1/psphot.config
r25660 r25727 1 1 2 BACKGROUND.XBIN S32 256# size of background superpixels3 BACKGROUND.YBIN S32 256# size of background superpixels2 BACKGROUND.XBIN S32 256 # size of background superpixels 3 BACKGROUND.YBIN S32 256 # size of background superpixels 4 4 5 5 SOFTEN.VARIANCE BOOL TRUE # XXX drop? soften the errors for bright pixels … … 12 12 PSF_CLUMP_GRID_SCALE F32 2.5 # XXX too large? size of Sx,Sy image pixel 13 13 14 PSF.RESIDUALS.RADIUS F32 9.0 15 PSF.RESIDUALS.SPATIAL_ORDER S32 1 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) 16 16 17 17 # PSF model parameters : choose the PSF model desired 18 18 PSF_MODEL STR PS_MODEL_PS1_V1 19 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights19 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights in CR stat 20 20 21 21 PSF.TREND.NX S32 3 … … 25 25 FULL_FIT_SN_LIM F32 25.0 26 26 27 APTREND.ORDER.MAX S32 327 APTREND.ORDER.MAX S32 3 28 28 29 DIAGNOSTIC.PLOTS 29 DIAGNOSTIC.PLOTS METADATA 30 30 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE 31 31 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 32 … … 33 33 END 34 34 35 DIFF 35 DIFF METADATA 36 36 BACKGROUND.XBIN S32 32 # size of background superpixels 37 37 BACKGROUND.YBIN S32 32 # size of background superpixels -
branches/eam_branches/20090715/ippconfig/isp/psphot.config
r15044 r25727 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 -
branches/eam_branches/20090715/ippconfig/lbc_red/psphot.config
r17154 r25727 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 -
branches/eam_branches/20090715/ippconfig/lulin/psphot.config
r18436 r25727 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 -
branches/eam_branches/20090715/ippconfig/megacam/psphot.config
r25022 r25727 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 -
branches/eam_branches/20090715/ippconfig/mosaic2/psphot.config
r25623 r25727 1 1 2 IMSTATS_NPIX S3210000 # number of pixels to use for sky estimate boxes:2 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 3 3 4 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 background5 SKY_STAT STR ROBUST_MEDIAN # statistic used to measure background 6 6 7 # PSF model parameters : choose the PSF model 8 # list as many PSF_MODEL options as desired 9 # if you want to list multiple entries, uncomment 'MULTI' here 10 # PSF_MODEL MULTI 7 PSF_MODEL STR PS_MODEL_QGAUSS 8 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 11 9 12 PSF_MODEL STR PS_MODEL_QGAUSS 13 # PSF_MODEL STR PS_MODEL_GAUSS 14 # PSF_MODEL STR PS_MODEL_PGAUSS 15 # 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 16 13 17 PSF_CLUMP_NX S32 1 # subdivide image in to NX x NY regions for 18 PSF_CLUMP_NY S32 3 # selecting PSF stars 14 # Mosaic 2 has substantial IQ variations in the y-direction 15 PSF.TREND.NX S32 1 16 PSF.TREND.NY S32 3 19 17 20 P SF_MAX_NSTARS S32 300 # limit number of stars used for PSF model21 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 22 20 23 PSF .TREND.MODE STR MAP24 PSF.TREND.NX S32 1 25 PSF.TREND.NY S32 3 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 26 24 27 PEAKS_NSIGMA_LIMIT F32 15.0 # peak significance threshold 28 MOMENTS_SN_MIN F32 10.0 # min S/N to measure moments 29 PSF_SN_LIM F32 20.0 # minimum S/N for stars used for PSF model 30 FULL_FIT_SN_LIM F32 10.0 31 EXT_MIN_SN F32 10.0 # fit galaxies above this S/N limit 32 AP_MIN_SN F32 10.0 25 EXT_MODEL STR PS_MODEL_QGAUSS 33 26 34 ## gene's overrides for testing: 35 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold 36 37 EXT_MODEL STR PS_MODEL_QGAUSS 38 39 PSF_MOMENTS_RADIUS F32 7 # calculate initial source moments with this radius 40 MOMENTS_MIN_PIXEL_SN F32 0.0 # XXX caution on this: too high and we will excessively clip 41 MOMENTS_GAUSS_SIGMA F32 2.0 # XXX TEST THIS: sigma in pixels (should be >> seeing equiv) 42 43 PSPHOT.EXT.NSIGMA.LIMIT F32 3.0 # sources with extNsigma greater that this get tagged as likely extended sources 44 PSPHOT.EXT.NSIGMA.MOMENTS F32 2.0 # sources with extNsigma greater that this get tagged as likely extended sources 45 46 EXTENDED_SOURCE_SN_LIM F32 3.0 27 EXTENDED_SOURCE_SN_LIM F32 3.0 47 28 #EXTENDED_SOURCE_ANALYSIS BOOL TRUE # perform any of the aperture-like measurements? 48 29 #EXTENDED_SOURCE_PETROSIAN BOOL TRUE 49 30 50 PSF.RESIDUALS.NSIGMA F32 3.0 # clip input stack of NSIGMA outliers 51 PSF.RESIDUALS.SPATIAL_ORDER S32 0 # fit spatial variations of the residuals at this order (0,1) 52 PSF.RESIDUALS.PIX.SN F32 0.0 # keep this pixel if residual is more significant than this 53 PSF.RESIDUALS.RADIUS F32 8.0 # keep this pixel if residual is more significant than this 54 55 MEASURE.APTREND BOOL TRUE 56 APTREND.ORDER.MAX S32 3 57 58 PSF_FIT_RADIUS F32 9.0 # fitting radius for test PSF model 31 # 3 to match PSF and Moments 2D variations 32 APTREND.ORDER.MAX S32 3 -
branches/eam_branches/20090715/ippconfig/sdss/psphot.config
r14644 r25727 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 -
branches/eam_branches/20090715/ippconfig/sdssmosaic/psphot.config
r24067 r25727 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 -
branches/eam_branches/20090715/ippconfig/simmosaic/psphot.config
r20889 r25727 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 -
branches/eam_branches/20090715/ippconfig/simple/psphot.config
r19320 r25727 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 -
branches/eam_branches/20090715/ippconfig/tek/psphot.config
r14564 r25727 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 -
branches/eam_branches/20090715/ippconfig/ucam/psphot.config
r12376 r25727 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 -
branches/eam_branches/20090715/ippconfig/uh8k/psphot.config
r18442 r25727 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 -
branches/eam_branches/20090715/ippconfig/vysos5/psphot.config
r20652 r25727 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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