Changeset 25766 for branches/eam_branches/20090820/ippconfig/sdssmosaic/psphot.config

Timestamp:

Oct 2, 2009, 5:10:19 PM (17 years ago)

Author:

eugene

Message:

merge changes from trunk

Location:

branches/eam_branches/20090820

Files:

• . (modified) (1 prop)
• ippconfig/sdssmosaic/psphot.config (modified) (3 diffs)

branches/eam_branches/20090820/ippconfig/sdssmosaic/psphot.config

@@ -1 @@
-
-# turn these on to see specific outputs
-SAVE.OUTPUT     BOOL    TRUE
-SAVE.BACKMDL    BOOL    TRUE
-#SAVE.RESID     BOOL    TRUE
-#SAVE.BACKGND   BOOL    TRUE
-SAVE.BACKSUB    BOOL    TRUE
-SAVE.PSF        BOOL    TRUE
-#LOAD.PSF       BOOL    FALSE
-#SAVE.PLOTS             BOOL    TRUE
-
-# for testing:
-# BREAK_POINT STR BACKMDL
-
 
 BACKGROUND.XBIN     S32  256            # size of background superpixels
 BACKGROUND.YBIN     S32  256            # size of background superpixels
 
-# image background parameters
-IMSTATS_NPIX        S32  10000           # number of pixels to use for sky estimate boxes:
-SKY_STAT            STR  FITTED_MEAN_V4  # statistic used to measure background
-SKY_CLIP_SIGMA      F32  2.0             # statistic used to measure background
-
-PEAKS_SMOOTH_SIGMA  F32   2.5            # smoothing kernel sigma in pixels
-PEAKS_NMAX          S32   5000           # on first pass, only keep NMAX peaks (0 == all)
-PEAKS_NSIGMA_LIMIT  F32   25.0           # peak significance threshold
-PEAKS_NSIGMA_LIMIT_2 F32   5.0           # peak significance threshold
-
-PSF_SN_LIM          F32  25              # minimum S/N for stars used for PSF model
-PSF_MAX_NSTARS      S32  300             # limit number of stars used for PSF model
+# what is the 2D variation of the SDSS PSF?
 PSF_CLUMP_NX        S32   3               # subdivide image in to NX x NY regions for 
 PSF_CLUMP_NY        S32   3               # selecting PSF stars
-PSF_MOMENTS_RADIUS  F32  12               # calculate initial source moments with this radius
+
+# test this:
 PSF_CLUMP_GRID_SCALE F32 2.5            # size of Sx,Sy image pixel
-
-PSF.RESIDUALS       BOOL  TRUE            # generate the residuals?
 
 # PSF model parameters : choose the PSF model desired
 PSF_MODEL           STR  PS_MODEL_PS1_V1
-PSPHOT.CR.NSIGMA.SOFTEN             F32   0.0025            # Softening parameter for weights
 
 # Use same default setting as in 2.6.1 (MAP is now global default)
@@ -45 +18 @@
 PSF.TREND.NY                        S32   0
 
-EXT_MIN_SN           F32  50.0           # fit galaxies above this S/N limit
-FULL_FIT_SN_LIM      F32  25.0
-MOMENTS_SN_MIN      F32    5.0
-AP_MIN_SN            F32   5.0
-
-OUTPUT.FORMAT        STR  PS1_V1
-
-PSF_SHAPE_NSIGMA     F32  3.0            # max significance for shape variation
-PSF_MAX_CHI          F32  50.0           # reject objects worse that this
-
-MEASURE.APTREND      BOOL TRUE           ### XXX for now, skip this (too many errors)
-APTREND.ORDER.MAX    S32  3
-
-# BREAK_POINT STR PASS1
-
+# match the SDSS radius:
 PSF_REF_RADIUS      F32  18.7            # aperture magnitudes are scaled via 
                                          # curve-of-growth to this radius
-
-DIAGNOSTIC.PLOTS                    METADATA
-  IMAGE.BACKGROUND.CELL.HISTOGRAM   BOOL  FALSE
-  IMAGE.BACKGROUND.CELL.HISTOGRAM.X S32   32
-  IMAGE.BACKGROUND.CELL.HISTOGRAM.Y S32   15
-END
-
-USE_FOOTPRINTS                      BOOL  TRUE            # use new pmFootprint peak packaging
-
-# Default is noap, nopsf; following recipes turn on one or both of these
-
+# for tests: Default is noap, nopsf; following recipes turn on one or both of these
 PSPHOT_NOAP_PSF METADATA
  PSF.TREND.MODE         STR     MAP
@@ -96 +45 @@
 END
 
+# put these values in the master?
 DIFF    METADATA
         BACKGROUND.XBIN     S32  32            # size of background superpixels