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: http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node190.html
Дата изменения: Tue Sep 20 19:45:18 2011 Дата индексирования: Mon Apr 11 02:47:21 2016 Кодировка: Поисковые слова: aurora |
The described procedure returns the one-dimensional response distribution in PI channels, based on an input energy.
CanonicalRedist retrieves a set of parameters from the EPIC-pn redistribution CCF and passes these to the CALPNALGO_resp routine. This routine then calculates the response, in each PI channel bin, for an input photon energy, an event pattern selection and a RAW-Y (row) position on the CCD.
The redistribution parameters have been calibrated as a function of: