Changeset 12376 for trunk/ippconfig/isp/psphot.config
- Timestamp:
- Mar 8, 2007, 9:28:54 PM (19 years ago)
- File:
-
- 1 edited
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trunk/ippconfig/isp/psphot.config (modified) (3 diffs)
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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
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