IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Ignore:
Timestamp:
Apr 4, 2011, 1:04:41 PM (15 years ago)
Author:
eugene
Message:

updates to pmPeak to better distinguish peak flux versions; updates to visualization; add bits for substantial suspect masking; consolidate assignment of source position and flux based on peak, moments, etc; improve footprint culling process; fix PSF_QF and PSF_QF_PERFECT calculations; fix source model chisq values

Location:
trunk/psModules
Files:
2 edited

Legend:

Unmodified
Added
Removed
  • trunk/psModules

    • Property svn:ignore
      •  

        old new  
        2828ChangeLog
        2929psmodules-*.tar.*
         30a.out.dSYM
  • trunk/psModules/src/objects/pmFootprint.h

    r30621 r31153  
    1010#ifndef PM_FOOTPRINT_H
    1111#define PM_FOOTPRINT_H
     12
     13// We need to choose up front if the culling algorithm uses the raw or smoothed image.
     14// depending on which we choose, we should produce sorted peaks based on peak->rawFlux or
     15// peak->smoothFlux
     16
     17# define PM_PEAKS_CULL_WITH_SMOOTHED_IMAGE 1
    1218
    1319typedef struct {
     
    8490                                 const float nsigma_delta, // how many sigma above local background a peak needs to be to survive
    8591                                 const float fPadding, // fractional padding added to stdev since bright peaks have unreasonably high significance
    86                                  const float min_threshold // minimum permitted coll height
     92                                 const float min_threshold, // minimum permitted coll height
     93                                 const float max_threshold,// maximum permitted coll height
     94                                 const bool isWeightVar // the input weight may be variance (sigma^2) or S/N (1/sigma)
    8795    );
    8896
Note: See TracChangeset for help on using the changeset viewer.