Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node152.html
Дата изменения: Fri Feb 23 12:57:25 1996 Дата индексирования: Tue Oct 2 17:50:37 2012 Кодировка: Поисковые слова: п п п п п п п п gemini |
The removal of unwanted spikes, above an otherwise featureless background such as the inter-order space of echelle spectra, is done most easily with a median filter. Therefore, in a first step a median filter is applied to the entire frame. This then enables the true background to be determined as described in Section `Background Definition' of this chapter. The subtraction of the background calculated completes the second step, and, as far as the inter-order space is concerned, the final result is reached already. The removal of cosmics from the object spectrum forms the third step and is restricted to the regions covered by the spectral orders in the background-corrected, but otherwise raw frame. This step comprises the following operations performed within a sliding (along and separately for each spectral order) window of user-specified width:
These three steps are the backbone of command FILTER/ECHELLE. The final output frame is the merger of the median-filtered inter-order domains with the spectral orders after having been subjected to step three. Note that the background has been subtracted already. A keyword BACKGROUND with contents SUBTRACTED is appended to the frame as a flag to subsequent high-level procedures so as not to have to go through the very time consuming step of the background modeling again. Delete that descriptor or change its contents if re-modeling of the residual background is desired.