Changeset 20557
- Timestamp:
- Nov 6, 2008, 2:39:59 AM (18 years ago)
- File:
-
- 1 edited
-
trunk/ippconfig/sdssmosaic/psphot.config (modified) (2 diffs)
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trunk/ippconfig/sdssmosaic/psphot.config
r20088 r20557 1 1 2 2 # turn these on to see specific outputs 3 SAVE.OUTPUT BOOL TRUE 3 4 SAVE.BACKMDL BOOL TRUE 5 #SAVE.RESID BOOL TRUE 4 6 #SAVE.BACKGND BOOL TRUE 5 #SAVE.BACKSUB BOOL TRUE 6 #SAVE.RESID BOOL TRUE 7 SAVE.BACKSUB BOOL TRUE 7 8 SAVE.PSF BOOL TRUE 8 SAVE.PLOTS BOOL TRUE 9 #LOAD.PSF BOOL FALSE 10 #SAVE.PLOTS BOOL TRUE 9 11 10 # image statistics parameters11 IMSTATS_NPIX S32 3000 # number of pixels to use for sky estimate boxes: 12 BACKGROUND.XBIN S32 256 # size of background superpixels 13 BACKGROUND.YBIN S32 256 # size of background superpixels 12 14 13 PSF_SN_LIM F32 10 # minimum S/N for stars used for PSF model 15 # image background parameters 16 IMSTATS_NPIX S32 10000 # number of pixels to use for sky estimate boxes: 17 SKY_STAT STR FITTED_MEAN_V4 # statistic used to measure background 18 SKY_CLIP_SIGMA F32 2.0 # statistic used to measure background 19 20 PEAKS_SMOOTH_SIGMA F32 2.5 # smoothing kernel sigma in pixels 21 PEAKS_NMAX S32 5000 # on first pass, only keep NMAX peaks (0 == all) 22 PEAKS_NSIGMA_LIMIT F32 25.0 # peak significance threshold 23 PEAKS_NSIGMA_LIMIT_2 F32 10.0 # peak significance threshold 24 25 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model 14 26 PSF_MAX_NSTARS S32 300 # limit number of stars used for PSF model 27 PSF_CLUMP_NX S32 3 # subdivide image in to NX x NY regions for 28 PSF_CLUMP_NY S32 3 # selecting PSF stars 29 PSF_MOMENTS_RADIUS F32 12 # calculate initial source moments with this radius 15 30 16 PSF_MODEL STR PS_MODEL_QGAUSS 17 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 22 # This is where aperture correction gets turned on and off - used to be false up to 2008-10-06 23 MEASURE.APTREND BOOL FALSE 24 PSF_CLUMP_NSIGMA F32 2.5 # region of Sx,Sy plane to use for selecting PSF stars 25 26 ## # PSFTREND must be a 2D polynomial 27 ## # the specified values are ignored but define the active components of the polynomial 28 ## PSF.TREND.MASK METADATA 29 ## NORDER_X S32 3 # number of x orders 30 ## NORDER_Y S32 3 # number of y orders 31 ## VAL_X00_Y00 F64 1 # polynomial coefficient 32 ## 33 ## VAL_X01_Y00 F64 1 # polynomial coefficient 34 ## VAL_X00_Y01 F64 1 # polynomial coefficient 35 ## 36 ## VAL_X02_Y00 F64 1 # polynomial coefficient 37 ## VAL_X01_Y01 F64 1 # polynomial coefficient 38 ## VAL_X00_Y02 F64 1 # polynomial coefficient 39 ## 40 ## VAL_X03_Y00 F64 1 # polynomial coefficient 41 ## VAL_X02_Y01 F64 1 # polynomial coefficient 42 ## VAL_X01_Y02 F64 1 # polynomial coefficient 43 ## VAL_X00_Y03 F64 1 # polynomial coefficient 44 ## NELEMENTS S32 10 # number of unmasked components 45 ## END # folder for 4D polynomial 31 # PSF model parameters : choose the PSF model desired 32 PSF_MODEL STR PS_MODEL_PS1_V1 46 33 47 34 # Use same default setting as in 2.6.1 (MAP is now global default) … … 50 37 PSF.TREND.NY S32 0 51 38 52 # Turn on variable PSF fitting - MAP tries to trade off between not having many stars and not having many bins. 53 # Try nx, ny up to 3 or 5. 54 # Note that MAP with NX, NY = 1 is the default in recipes/psphot.config now! 55 # PSF.TREND.MODE STR MAP 56 # PSF.TREND.NX S32 5 57 # PSF.TREND.NY S32 5 39 MOMENTS_SN_MIN F32 30.0 40 EXT_MIN_SN F32 50.0 # fit galaxies above this S/N limit 41 FULL_FIT_SN_LIM F32 50.0 42 AP_MIN_SN F32 50.0 58 43 59 XMIN F32 15 44 OUTPUT.FORMAT STR PS1_DEV_1 60 45 61 PSF.RESIDUALS BOOL true 62 PSF.RESIDUALS.SPATIAL_ORDER S32 1 46 PSF_SHAPE_NSIGMA F32 3.0 # max significance for shape variation 47 PSF_MAX_CHI F32 50.0 # reject objects worse that this 48 APTREND.ORDER.MAX S32 1 63 49 64 # The parameter BREAK_POINT stopped the analysis after first linear 65 # fit to sources. Should be NONE or commented out. 66 # BREAK_POINT STR ENSEMBLE 67 OUTPUT.FORMAT STR PS1_DEV_1 50 MEASURE.APTREND BOOL TRUE ### XXX for now, skip this (too many errors) 51 # BREAK_POINT STR PASS1 68 52 69 PSPHOT.SUMMIT METADATA 70 PEAKS_SMOOTH_SIGMA F32 0.8 # peak significance threshold 71 PEAKS_NSIGMA_LIMIT F32 50.0 # peak significance threshold 72 PEAKS_NMAX S32 1000 73 SAVE.RESID BOOL FALSE 74 PSF_SN_LIM F32 25 # minimum S/N for stars used for PSF model 75 MOMENTS_SN_MIN F32 25.0 76 PSF_MODEL STR PS_MODEL_PGAUSS 53 PSF_REF_RADIUS F32 18.7 # aperture magnitudes are scaled via 54 # curve-of-growth to this radius 55 56 DIAGNOSTIC.PLOTS METADATA 57 IMAGE.BACKGROUND.CELL.HISTOGRAM BOOL FALSE 58 IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32 32 59 IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32 15 77 60 END 78 61 79 # Turn on use of footprints to avoid objectcs being found in 80 # diffraction spikes etc. of bright stars 81 USE_FOOTPRINTS BOOL T # use new pmFootprint peak packaging 62 USE_FOOTPRINTS BOOL TRUE # use new pmFootprint peak packaging 82 63 83 # Set aperture correction radius to same 7.4" as SDSS (see EDR paper) 84 PSF_REF_RADIUS F32 18.7 # aperture magnitudes are scaled via 85 # curve-of-growth to this radius 64 # Default is noap, nopsf; following recipes turn on one or both of these 65 66 PSPHOT_NOAP_PSF METADATA 67 PSF.TREND.MODE STR MAP 68 PSF.TREND.NX S32 3 69 PSF.TREND.NY S32 3 70 MEASURE.APTREND BOOL FALSE 71 END 72 73 PSPHOT_AP_NOPSF METADATA 74 PSF.TREND.MODE STR POLY_ORD 75 PSF.TREND.NX S32 0 76 PSF.TREND.NY S32 0 77 MEASURE.APTREND BOOL TRUE 78 END 79 80 PSPHOT_AP_PSF METADATA 81 PSF.TREND.MODE STR MAP 82 PSF.TREND.NX S32 3 83 PSF.TREND.NY S32 3 84 MEASURE.APTREND BOOL TRUE 85 END 86
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