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: http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node597.html Дата изменения: Tue Sep 20 19:45:20 2011 Дата индексирования: Mon Apr 11 03:12:57 2016 Кодировка: Поисковые слова: asteroid | 
 
 
 
 
 
 
 
  
| ZPTU | zero point of U-filter | 
| ZPTB | zero point of B-filter | 
| ZPTV | zero point of V-filter | 
| ZPTUW1 | zero point of UW1-filter | 
| ZPTUM2 | zero point of UM2-filter | 
| ZPTUW2 | zero point of UW2-filter | 
| ZPTMAGNI | zero point of magnifier | 
| ZPTWHITE | zero point of white light-filter | 
The count rates conversion is made with the assumption that the full PSF is sampled. In case of partial PSF sampling the magnitudes have to be corrected by the calling task.
The transformation of the input count rate  into the natural system
 
into the natural system  (in units of magnitude)  
is described by the equation:
 (in units of magnitude)  
is described by the equation: 
|  | (36) | 
 is the zero point of the used filter.
 is the zero point of the used filter.
The original routine has been aliased as CAL_omNaturalMagnitude.
 
 
 
 
 
 
