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: http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node905.html
Дата изменения: Tue Sep 20 19:45:21 2011 Дата индексирования: Mon Apr 11 03:58:58 2016 Кодировка: Поисковые слова: о п п |
This step is done mostly interactively and uses some basic ad-hoc IDL procedures, mainly for testing and checking of the consistency of the results.Once the observations have been selected and the count spectra extracted, the available spectra of each background level are accumulated. The combined spectrum is built as follows