Changeset 12376
- Timestamp:
- Mar 8, 2007, 9:28:54 PM (19 years ago)
- Location:
- trunk/ippconfig
- Files:
-
- 4 edited
-
ctio_mosaic2/psphot.config (modified) (1 diff)
-
isp/psphot.config (modified) (3 diffs)
-
megacam/psphot.config (modified) (4 diffs)
-
ucam/psphot.config (modified) (3 diffs)
Legend:
- Unmodified
- Added
- Removed
-
trunk/ippconfig/ctio_mosaic2/psphot.config
r10871 r12376 1 1 2 # t hese options turn on different inputs and/oroutputs3 SAVE.BACKMDL BOOL FALSE4 SAVE.BACKGND BOOL FALSE5 SAVE.BACKSUB BOOL FALSE2 # turn these on to see specific outputs 3 #SAVE.BACKMDL BOOL TRUE 4 #SAVE.BACKGND BOOL TRUE 5 #SAVE.BACKSUB BOOL TRUE 6 6 SAVE.RESID BOOL TRUE 7 SAVE.PSF BOOL FALSE 8 LOAD.PSF BOOL FALSE 9 SAVE.PLOTS BOOL TRUE 7 #SAVE.PSF BOOL TRUE 8 #LOAD.PSF BOOL FALSE 10 9 11 # the zero point is used to set a basic scale for DVO 12 # XXX it may not currently be read : double check this (EAM) 13 ZERO_POINT F32 25.000 # zero point used by DVO 10 IMSTATS_NPIX S32 1000 # number of pixels to use for sky estimate boxes: 14 11 15 # these parameter govern how the background is measured 16 BACKGROUND_XBIN S32 128 # size of background superpixels 17 BACKGROUND_YBIN S32 128 # size of background superpixels 18 IMSTATS_NPIX S32 2000 # number of pixels to use for sky estimate boxes: 19 20 SKY_BIAS F32 0.0 # offset applied to measured sky (FOR TESTING) 21 SKY_FIT_ORDER S32 0 22 SKY_FIT_LINEAR BOOL FALSE 23 SKY_STAT STR FITTED_MEAN # statistic used to measure background 24 # allowed values for SKY_STAT: 25 # SAMPLE_MEAN, SAMPLE_MEDIAN, CLIPPED_MEAN, ROBUST_MEAN, ROBUST_QUARTILE, FITTED_MEAN 26 27 # masking parameters (XXX EAM : rework this to use psRegion like ANALYSIS_REGION) 28 XMIN F32 0 # minimum valid x-coord 29 XMAX F32 0 # maximum valid x-coord 30 YMIN F32 0 # minimum valid y-coord 31 YMAX F32 0 # maximum valid y-coord 32 SATURATION F32 64000 # saturation level on this chip 33 34 # peak finding 35 PEAKS_SMOOTH_SIGMA F32 1.0 # smoothing kernel sigma in pixels 36 PEAKS_SMOOTH_NSIGMA F32 2.0 # smoothing kernel width in sigmas 37 PEAKS_NSIGMA_LIMIT F32 50.0 # peak significance threshold 38 39 # parameters to control the selection of the peak in the Sx,Sy plane 40 MOMENTS_SCALE F32 0.1 41 MOMENTS_SN_MIN F32 10.0 42 MOMENTS_SX_MAX F32 3.0 43 MOMENTS_SY_MAX F32 3.0 44 MOMENTS_AR_MAX F32 1.5 # maximum axial ratio: 1 / AR < (sx / sy) < AR 45 46 # basic object statistics 47 SKY_INNER_RADIUS F32 15 # square annulus for local sky measurement 48 SKY_OUTER_RADIUS F32 25 # square annulus for local sky measurement 49 PSF_MOMENTS_RADIUS F32 3 # calculate initial source moments with this radius 50 PSF_SN_LIM F32 50 # minimum S/N for stars used for PSF model 12 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model 51 13 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 52 14 53 15 # PSF model parameters : choose the PSF model 54 16 # list as many PSF_MODEL options as desired 17 # if you want to list multiple entries, uncomment 'MULTI' here 55 18 # PSF_MODEL MULTI 56 PSF_MODEL STR PS_MODEL_GAUSS 19 PSF_MODEL STR PS_MODEL_QGAUSS 20 # PSF_MODEL STR PS_MODEL_GAUSS 57 21 # PSF_MODEL STR PS_MODEL_PGAUSS 58 # PSF_MODEL STR PS_MODEL_QGAUSS59 22 # PSF_MODEL STR PS_MODEL_TGAUSS ## not well tested, not very successful 60 23 61 # PSF.TREND.MASK must be a 2D polynomial 62 # the specified values are ignored but define the active components of the polynomial 63 PSF.TREND.MASK METADATA 64 NORDER_X S32 2 # number of x orders 65 NORDER_Y S32 2 # number of y orders 66 VAL_X00_Y00 F64 1 # polynomial coefficient 67 VAL_X01_Y00 F64 1 # polynomial coefficient 68 VAL_X00_Y01 F64 1 # polynomial coefficient 69 VAL_X02_Y00 F64 1 # polynomial coefficient 70 VAL_X01_Y01 F64 1 # polynomial coefficient 71 VAL_X00_Y02 F64 1 # polynomial coefficient 72 NELEMENTS S32 6 # number of unmasked components 73 END # folder for 2D polynomial 74 75 PSF_FIT_RADIUS F32 15.0 # fitting radius for test PSF model 76 PSF_REF_RADIUS F32 25.0 # aperture magnitudes are scaled via 77 # curve-of-growth to this radius 78 # PSF-like source model parameters 79 PSF_FIT_NSIGMA F32 1.0 # significance for pixel included in fit 80 PSF_FIT_PADDING F32 2.0 # extra annulus to use for fit 81 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation 82 PSF_MIN_SN F32 2.0 # reject objects below this significance 83 PSF_MAX_CHI F32 50.0 # reject objects worse that this 84 FULL_FIT_SN_LIM F32 10.0 85 86 # EXTended source model parameters 87 EXT_MODEL STR PS_MODEL_PGAUSS 24 MOMENTS_SN_MIN F32 20.0 # min S/N to measure moments 88 25 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 89 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit 90 EXT_FIT_PADDING F32 5 # extra annulus to use for fit 91 EXT_MOMENTS_RADIUS F32 9 92 93 FITMODE STR BLEND 94 DEBLEND_PEAK_FRACTION F32 0.1 95 DEBLEND_SKY_NSIGMA F32 10.0 96 97 # APTREND STR NONE, CONSTANT, SKYBIAS, SKYSAT, XY_LIN, SKY_XY_LIN, SKYSAT_XY_LIN, ALL 98 APTREND STR CONSTANT 26 FULL_FIT_SN_LIM F32 50.0 99 27 AP_MIN_SN F32 25.0 100 101 # test options102 # BREAK_POINT may be one of (PEAKS, MOMENTS, PSFMODEL, ENSEMBLE)103 # BREAK_POINT STR MOMENTS104 # PEAKS_OUTPUT_FILE STR peaks.dat105 # MOMENTS_OUTPUT_FILE STR moments.dat106 # ANALYSIS_REGION STR [1000:1600,2800:3400]107 # POISSON_ERRORS BOOL TRUE108 109 # optional parameter to limit the actual analysis to a fraction of the image110 # do not uncomment this in the master psphot.config file111 # ANALYSIS_REGION STR [1000:1600,2800:3400]112 113 IGNORE_GROWTH BOOL FALSE114 CONSTANT_PHOTOMETRIC_WEIGHTS BOOL TRUE # Should the photometric code [currently only ensemblePSF] refuse to weight each pixel by it's significance?115 INTERPOLATE_AP BOOL TRUE116 POISSON_ERRORS BOOL TRUE -
trunk/ippconfig/isp/psphot.config
r11573 r12376 1 1 2 SAVE.OUTPUT BOOL TRUE 2 # turn these on to see specific outputs 3 3 #SAVE.BACKMDL BOOL TRUE 4 4 #SAVE.BACKGND BOOL TRUE … … 7 7 #SAVE.PSF BOOL TRUE 8 8 9 #LOAD.PSF BOOL FALSE10 11 # image noise parameters12 RDNOISE STR HD:RDNOISE # read-noise in electrons13 GAIN STR HD:GAIN # electrons / DN14 ZERO_POINT F32 25.000 # zero point used by DVO15 16 # background model :17 BACKGROUND.XBIN S32 12818 BACKGROUND.YBIN S32 12819 20 # masking parameters21 XMIN F32 2 # minimum valid x-coord22 XMAX F32 -2 # maximum valid x-coord23 YMIN F32 2 # minimum valid y-coord24 YMAX F32 -2 # maximum valid y-coord25 SATURATION F32 50000 # saturation level on this chip26 MIN_VALID_PIXEL F32 1 # saturation level on this chip27 28 9 # image statistics parameters 29 10 IMSTATS_NPIX S32 1000 # number of pixels to use for sky estimate boxes: 30 11 31 # peak finding32 PEAKS_SMOOTH_SIGMA F32 1.0 # smoothing kernel sigma in pixels33 PEAKS_SMOOTH_NSIGMA F32 3.0 # smoothing kernel width in sigmas34 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold35 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold36 37 # basic object statistics38 SKY_INNER_RADIUS F32 15 # square annulus for local sky measurement39 SKY_OUTER_RADIUS F32 25 # square annulus for local sky measurement40 PSF_MOMENTS_RADIUS F32 3 # calculate initial source moments with this radius41 12 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model 42 PSF_CLUMP_NSIGMA F32 3 # size of PSF clump in image (use a larger number for images with large PSF variations)43 13 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 44 14 … … 51 21 # PSF_MODEL STR PS_MODEL_TEST1 52 22 53 MOMENTS_SCALE F32 0.154 23 MOMENTS_SN_MIN F32 10.0 55 MOMENTS_SX_MAX F32 3.056 MOMENTS_SY_MAX F32 3.057 MOMENTS_AR_MAX F32 5.0 # maximum axial ratio: 1 / AR < (sx / sy) < AR58 59 PSF_FIT_RADIUS F32 9.0 # fitting radius for test PSF model60 PSF_REF_RADIUS F32 11.0 # aperture magnitudes are scaled via61 # curve-of-growth to this radius62 # PSF-like source model parameters63 PSF_FIT_NSIGMA F32 1.0 # significance for pixel included in fit64 PSF_FIT_PADDING F32 2.0 # extra annulus to use for fit65 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation66 PSF_MIN_SN F32 2.0 # reject objects below this significance67 PSF_MAX_CHI F32 50.0 # reject objects worse than this68 69 # EXTended source model parameters70 EXT_MODEL STR PS_MODEL_PGAUSS71 24 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 72 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit73 EXT_FIT_PADDING F32 10 # extra annulus to use for fit74 EXT_MOMENTS_RADIUS F32 975 76 FITMODE STR BLEND77 DEBLEND_PEAK_FRACTION F32 0.178 DEBLEND_SKY_NSIGMA F32 10.079 80 # APTREND STR CONSTANT81 APTREND STR ALL82 # APTREND STR SKYSAT_XY_LIN83 # APTREND STR SKYSAT84 # APTREND STR SKYBIAS85 APTREND.XORDER S32 286 APTREND.YORDER S32 287 25 FULL_FIT_SN_LIM F32 50.0 88 26 AP_MIN_SN F32 20.0 89 MAX_AP_OFFSET F32 0.590 CONSTANT_PHOTOMETRIC_WEIGHTS BOOL TRUE # Should the photometric code [currently only ensemblePSF]91 # refuse to weight each pixel by it's significance?92 93 # test options94 95 # BREAK_POINT may be one of (PEAKS, MOMENTS, PSFMODEL, ENSEMBLE)96 BREAK_POINT STR ENSEMBLE97 98 # PEAKS_OUTPUT_FILE STR peaks.dat99 # MOMENTS_OUTPUT_FILE STR moments.dat100 # ANALYSIS_REGION STR [1000:1600,2800:3400]101 # POISSON_ERRORS BOOL TRUE102 # SKY_BIAS F32 0.0103 27 104 28 # PSFTREND must be a 2D polynomial -
trunk/ippconfig/megacam/psphot.config
r7532 r12376 7 7 #LOAD.PSF BOOL FALSE 8 8 9 # image noise parameters10 RDNOISE STR HD:RDNOISE # read-noise in electrons11 GAIN STR HD:GAIN # electrons / DN12 ZERO_POINT F32 25.000 # zero point used by DVO13 14 # background model :15 BACKGROUND.XBIN S32 12816 BACKGROUND.YBIN S32 12817 18 9 # masking parameters 19 10 XMIN F32 2 # minimum valid x-coord … … 21 12 YMIN F32 2 # minimum valid y-coord 22 13 YMAX F32 -2 # maximum valid y-coord 23 SATURATION F32 50000 # saturation level on this chip24 MIN_VALID_PIXEL F32 1 # saturation level on this chip25 14 26 15 # image statistics parameters 27 16 IMSTATS_NPIX S32 1000 # number of pixels to use for sky estimate boxes: 28 17 29 # peak finding30 PEAKS_SMOOTH_SIGMA F32 1.0 # smoothing kernel sigma in pixels31 PEAKS_SMOOTH_NSIGMA F32 3.0 # smoothing kernel width in sigmas32 # PEAKS_NSIGMA_LIMIT F32 10.0 # peak significance threshold33 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold34 35 # basic object statistics36 SKY_INNER_RADIUS F32 15 # square annulus for local sky measurement37 SKY_OUTER_RADIUS F32 25 # square annulus for local sky measurement38 PSF_MOMENTS_RADIUS F32 3 # calculate initial source moments with this radius39 18 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model 40 19 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model … … 42 21 # PSF model parameters : choose the PSF model 43 22 # list as many PSF_MODEL options as desired 23 # if you want to list multiple entries, uncomment 'MULTI' here 44 24 # PSF_MODEL MULTI 45 25 PSF_MODEL STR PS_MODEL_QGAUSS … … 48 28 # PSF_MODEL STR PS_MODEL_TGAUSS ## not well tested, not very successful 49 29 50 MOMENTS_SCALE F32 0.151 30 MOMENTS_SN_MIN F32 30.0 52 MOMENTS_SX_MAX F32 3.053 MOMENTS_SY_MAX F32 3.054 MOMENTS_AR_MAX F32 1.5 # maximum axial ratio: 1 / AR < (sx / sy) < AR55 56 PSF_FIT_RADIUS F32 15.0 # fitting radius for test PSF model57 PSF_REF_RADIUS F32 25.0 # aperture magnitudes are scaled via58 59 # PSF-like source model parameters60 PSF_FIT_NSIGMA F32 1.0 # significance for pixel included in fit61 PSF_FIT_PADDING F32 5.0 # extra annulus to use for fit62 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation63 PSF_MIN_SN F32 2.0 # reject objects below this significance64 PSF_MAX_CHI F32 50.0 # reject objects worse that this65 66 # EXTended source model parameters67 EXT_MODEL STR PS_MODEL_PGAUSS68 31 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 69 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit70 EXT_FIT_PADDING F32 5 # extra annulus to use for fit71 EXT_MOMENTS_RADIUS F32 972 73 FITMODE STR BLEND74 DEBLEND_PEAK_FRACTION F32 0.175 DEBLEND_SKY_NSIGMA F32 10.076 77 APTREND STR SKYSAT78 32 FULL_FIT_SN_LIM F32 50.0 79 33 AP_MIN_SN F32 50.0 80 34 81 # BREAK_POINT STR PEAKS82 # PEAKS_OUTPUT_FILE STR peaks.dat83 # MOMENTS_OUTPUT_FILE STR moments.dat84 # ANALYSIS_REGION STR [1000:1600,2800:3400] -
trunk/ippconfig/ucam/psphot.config
r8825 r12376 1 1 2 # turn these on to see specific outputs 2 3 #SAVE.BACKMDL BOOL TRUE 3 4 #SAVE.BACKGND BOOL TRUE 4 5 #SAVE.BACKSUB BOOL TRUE 5 #SAVE.RESID BOOL TRUE6 SAVE.RESID BOOL TRUE 6 7 #SAVE.PSF BOOL TRUE 7 8 #LOAD.PSF BOOL FALSE 8 9 9 # image noise parameters10 RDNOISE STR HD:RDNOISE # read-noise in electrons11 GAIN STR HD:GAIN # electrons / DN12 ZERO_POINT F32 25.000 # zero point used by DVO13 14 # background model :15 BACKGROUND.XBIN S32 12816 BACKGROUND.YBIN S32 12817 18 # masking parameters19 XMIN F32 2 # minimum valid x-coord20 XMAX F32 -2 # maximum valid x-coord21 YMIN F32 2 # minimum valid y-coord22 YMAX F32 -2 # maximum valid y-coord23 SATURATION F32 50000 # saturation level on this chip24 MIN_VALID_PIXEL F32 1 # saturation level on this chip25 26 # image statistics parameters27 10 IMSTATS_NPIX S32 1000 # number of pixels to use for sky estimate boxes: 28 11 29 # peak finding30 PEAKS_SMOOTH_SIGMA F32 1.0 # smoothing kernel sigma in pixels31 PEAKS_SMOOTH_NSIGMA F32 3.0 # smoothing kernel width in sigmas32 # PEAKS_NSIGMA_LIMIT F32 10.0 # peak significance threshold33 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold34 35 # basic object statistics36 SKY_INNER_RADIUS F32 15 # square annulus for local sky measurement37 SKY_OUTER_RADIUS F32 25 # square annulus for local sky measurement38 PSF_MOMENTS_RADIUS F32 3 # calculate initial source moments with this radius39 12 PSF_SN_LIM F32 100 # minimum S/N for stars used for PSF model 40 13 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model … … 42 15 # PSF model parameters : choose the PSF model 43 16 # list as many PSF_MODEL options as desired 17 # if you want to list multiple entries, uncomment 'MULTI' here 44 18 # PSF_MODEL MULTI 45 19 PSF_MODEL STR PS_MODEL_QGAUSS … … 48 22 # PSF_MODEL STR PS_MODEL_TGAUSS ## not well tested, not very successful 49 23 50 MOMENTS_SCALE F32 0.1 51 MOMENTS_SN_MIN F32 30.0 52 MOMENTS_SX_MAX F32 3.0 53 MOMENTS_SY_MAX F32 3.0 54 MOMENTS_AR_MAX F32 1.5 # maximum axial ratio: 1 / AR < (sx / sy) < AR 55 56 PSF_FIT_RADIUS F32 15.0 # fitting radius for test PSF model 57 PSF_REF_RADIUS F32 25.0 # aperture magnitudes are scaled via 58 59 # PSF-like source model parameters 60 PSF_FIT_NSIGMA F32 1.0 # significance for pixel included in fit 61 PSF_FIT_PADDING F32 5.0 # extra annulus to use for fit 62 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation 63 PSF_MIN_SN F32 2.0 # reject objects below this significance 64 PSF_MAX_CHI F32 50.0 # reject objects worse that this 65 66 # EXTended source model parameters 67 EXT_MODEL STR PS_MODEL_PGAUSS 24 MOMENTS_SN_MIN F32 20.0 # min S/N to measure moments 68 25 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 69 EXT_FIT_NSIGMA F32 1 # significance for pixel included in fit70 EXT_FIT_PADDING F32 5 # extra annulus to use for fit71 EXT_MOMENTS_RADIUS F32 972 73 FITMODE STR BLEND74 DEBLEND_PEAK_FRACTION F32 0.175 DEBLEND_SKY_NSIGMA F32 10.076 77 APTREND STR SKYSAT78 26 FULL_FIT_SN_LIM F32 50.0 79 AP_MIN_SN F32 50.0 80 81 # BREAK_POINT STR PEAKS 82 # PEAKS_OUTPUT_FILE STR peaks.dat 83 # MOMENTS_OUTPUT_FILE STR moments.dat 84 # ANALYSIS_REGION STR [1000:1600,2800:3400] 27 AP_MIN_SN F32 25.0
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