Changeset 25660
- Timestamp:
- Sep 29, 2009, 10:08:56 AM (17 years ago)
- File:
-
- 1 edited
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branches/eam_branches/20090715/ippconfig/gpc1/psphot.config
r25623 r25660 1 1 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE 4 SAVE.BACKMDL BOOL TRUE 5 SAVE.BACKGND BOOL TRUE 6 SAVE.BACKSUB BOOL TRUE 7 SAVE.PSF BOOL TRUE 8 SAVE.PLOTS BOOL TRUE 2 BACKGROUND.XBIN S32 256 # size of background superpixels 3 BACKGROUND.YBIN S32 256 # size of background superpixels 9 4 10 BACKGROUND.XBIN S32 256 # size of background superpixels 11 BACKGROUND.YBIN S32 256 # size of background superpixels 12 13 # image background parameters 14 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 15 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background 16 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background 17 18 # soften the errors for bright pixels: 19 SOFTEN.VARIANCE BOOL TRUE 5 SOFTEN.VARIANCE BOOL TRUE # XXX drop? soften the errors for bright pixels 20 6 SOFTEN.VARIANCE.FRACTION F32 0.005 21 7 22 PEAKS_SMOOTH_SIGMA F32 2.5 # smoothing kernel sigma in pixels 23 PEAKS_NMAX S32 5000 # on first pass, only keep NMAX peaks (0 == all) 24 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold 25 PEAKS_NSIGMA_LIMIT_2 F32 5.0 # peak significance threshold 8 PEAKS_SMOOTH_SIGMA F32 2.5 # smoothing kernel sigma in pixels 26 9 27 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model 28 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 29 PSF_CLUMP_NX S32 3 # subdivide image in to NX x NY regions for 30 PSF_CLUMP_NY S32 3 # selecting PSF stars 31 PSF_MOMENTS_RADIUS F32 12 # calculate initial source moments with this radius 32 PSF_CLUMP_GRID_SCALE F32 2.5 # size of Sx,Sy image pixel 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 33 13 34 PSF.RESIDUALS BOOL TRUE # generate the residuals? 35 PSF.RESIDUALS.PIX.SN F32 0.0 # keep this pixel if residual is more significant than this 36 PSF.RESIDUALS.RADIUS F32 9.0 # keep this pixel if residual is more significant than this 37 PSF.RESIDUALS.SPATIAL_ORDER S32 1 # fit spatial variations of the residuals at this order (0,1) 38 # PSF.RESIDUALS BOOL FALSE # 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) 39 16 40 17 # PSF model parameters : choose the PSF model desired 41 PSF_MODEL STRPS_MODEL_PS1_V118 PSF_MODEL STR PS_MODEL_PS1_V1 42 19 PSPHOT.CR.NSIGMA.SOFTEN F32 0.0025 # Softening parameter for weights 43 20 44 PSF.TREND.MODE STR MAP # other options: POLY_CHEB, POLY_ORD45 21 PSF.TREND.NX S32 3 46 22 PSF.TREND.NY S32 3 47 23 48 PSF_FIT_RADIUS_SCALE F32 7.0 # fitting radius for test PSF model 49 PSF_APERTURE_SCALE F32 4.0 # fitting radius for test PSF model 24 # rename NONLINEAR_FIT_SN_LIM? 25 FULL_FIT_SN_LIM F32 25.0 50 26 51 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 52 FULL_FIT_SN_LIM F32 25.0 53 MOMENTS_SN_MIN F32 5.0 54 AP_MIN_SN F32 5.0 55 56 OUTPUT.FORMAT STR PS1_V2 57 58 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation 59 PSF_MAX_CHI F32 50.0 # reject objects worse that this 60 61 MEASURE.APTREND BOOL TRUE ### XXX for now, skip this (too many errors) 62 APTREND.ORDER.MAX S32 3 27 APTREND.ORDER.MAX S32 3 63 28 64 29 DIAGNOSTIC.PLOTS METADATA … … 68 33 END 69 34 70 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging71 72 35 DIFF METADATA 73 BACKGROUND.XBINS32 32 # size of background superpixels74 BACKGROUND.YBINS32 32 # size of background superpixels36 BACKGROUND.XBIN S32 32 # size of background superpixels 37 BACKGROUND.YBIN S32 32 # size of background superpixels 75 38 END
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