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: http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node183.html
Дата изменения: Tue Sep 20 19:45:18 2011 Дата индексирования: Mon Apr 11 02:46:52 2016 Кодировка: Поисковые слова: observatory |
The described procedure returns the one-dimensional response distribution in PI channels, based on an input energy. The redistribution function of the MOS cameras comprises a main peak (roughly centred on the input photon energy); a lower-energy secondary peak, whose relative magnitude is inversely correlated with the photon energy, and a noise term which extends down to the detection threshold energy. Details of the current calculation are given in the CCF release note, CAL-SRN-272.
CanonicalRedist retrieves a set of parameters from the appropriate MOS redistribution CCF and passes these to the CALMOSALGO initialisation routine CALMOSALGO_initRmfRow. The routine CALMOSALGO_rmfRow may then be used to calculate the response, in each PI channel bin, for a given input energy and event pattern selection.
The redistribution parameters have been calibrated as a function of: