- Timestamp:
- Dec 22, 2010, 6:28:58 AM (15 years ago)
- File:
-
- 1 edited
Legend:
- Unmodified
- Added
- Removed
-
branches/eam_branches/ipp-20101205/psModules/src/objects/pmSource.h
r30139 r30142 54 54 pmPeak *peak; ///< Description of peak pixel. 55 55 psImage *pixels; ///< Rectangular region including object pixels. 56 psImage *variance; ///< Image variance.56 psImage *variance; ///< Image variance. 57 57 psImage *maskObj; ///< unique mask for this object which marks included pixels associated with objects. 58 58 psImage *maskView; ///< view into global image mask for this object region 59 59 psImage *modelFlux; ///< cached copy of the best model for this source 60 psImage *psfImage; ///< cached copy of the psf model for this source60 psImage *psfImage; ///< cached copy of the psf model for this source 61 61 pmMoments *moments; ///< Basic moments measured for the object. 62 62 pmModel *modelPSF; ///< PSF Model fit (parameters and type) … … 90 90 pmSourceDiffStats *diffStats; ///< extra parameters for difference detections 91 91 psArray *radialAper; ///< radial flux in circular apertures 92 pmSource *parent; ///< reference to the master source from which this is derived 92 93 int imageID; 93 94 }; 95 96 /* a pmSource is the information about a (possible) blob of flux in a specific image. A source 97 * may represent an insignificant or undetected source. There may be multiple representations 98 * of an image (eg, alternate smoothed copies); sources on alternate images may have a pointer 99 * to the version on the primary image (source->parent). A set of sources on different, but 100 * related images (eg, multiple exposures or different filters) which (may) represent the same 101 * astronomical object are grouped together with the pmPhotObj type (set pmPhotObj.h). 102 * 103 * A single source may be fitted with multiple models (not at the same time!). The PSF model 104 * fit is a fit of the position (optionally) and the flux to the PSF model at the location of 105 * the source. Alternate model fits are extended source models. The best model fit is used to 106 * subtract the object from the image. 107 */ 94 108 95 109 /** pmPSFClump data structure
Note:
See TracChangeset
for help on using the changeset viewer.
