... to 0 The low-energy redistribution is being recalibrated based on RGS models of line-rich sources (1E0102-72, Zeta Puppis, and the comet C/2000 WM1) These results are included in a new version of the redistribution calibration file to be distributed soon ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201003/minutes-cal-2010.pdf -- 66.3 Кб -- 13.05.2014 Похожие документы
... parameter are being refined, using RGS-based models of deep observations of line rich sources: a) 1E0102.2-7219 (especially strong and well separated O and Ne emission lines); b) Zeta Puppis (strong N lines); c) Comet C/2000 WM1 (strong N and C lines ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200904/Minutes-cal-000409.pdf -- 92.0 Кб -- 13.05.2014 Похожие документы