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: http://xmm.vilspa.esa.es/external/xmm_sw_cal/calib/updates/update-20030129.shtml
Дата изменения: Unknown Дата индексирования: Wed Apr 13 13:05:50 2016 Кодировка: Поисковые слова: п п п п п п п п п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п р п |
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The canned MOS RMFs are observing mode and observation date dependent. The files are called; | |
m<camera><ccd>_<version>_<mode>_<patterns>_<start_date>.rmf |
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For example; | |
m11_r7_im_all_2000-11-09.rmf m11_r7_im_all_2001-04-18.rmf |
<camera> | 1 or 2 for MOS-1 and MOS-2 |
<ccd> | The number of the CCD, only the central CCD (number 1) is available at the moment. The variation between CCD s is small. |
<version> | Version number, currently 'r7' |
<mode> | 'im' for all imaging modes, 'ti' for Timing mode. |
<patterns> | 'p0' for pattern 0 only, 'all' for patterns 0 - 12 |
<start_date> | The first observation date for which this file should be used. The last observation date is given by the sta rt date of the next file in the sequence, e.g. m11_r7_im_all_2000-11-09.rmf should be used for observation dates fro m 09/11/2000 to 17/04/2001 inclusive. |
epn_ff20_dY9_medium.rmf | doubles selected from CCD lines 180-199, medium filter |
epn_ff20_dY9_thick.rmf | same, thick filter |
epn_ff20_dY9_thin.rmf | same, thin filter |
epn_ff20_dY9_closed.rmf | same, no filter, no telescope areas (useful for cal source) |
epn_ff20_dY9.rmf |
same, pure redistribution, normalised to 1, without double fraction applied. Read also this update. |
epn_ff20_sY9_medium.rmf | singles selected from CCD lines 180-199, medium filter |
epn_ff20_sdY9_medium.rmf | singles+doubles from CCD lines 180-199, medium filter |