... Astrophysical Sources From previous results: Analysis of line width trends at Fe-K energies of SNR N132D and EtaCarinae (F. Haberl, 2010) do not confirm the time dependence of the energy resolution seen in the calibration source. ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/smith-cal-2012-2.pdf -- 710.9 Кб -- 13.05.2014 Похожие документы
... Med energies 1E0102, High energies (resolution) EtaCarinae · Low energies: o No ... up effects High energies: o Etacarinae observation in same binary orbital phase (5 ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200605/MinutesCAL0605mpe.pdf -- 135.1 Кб -- 14.05.2014 Похожие документы
... CTI/Gain (KD, MK by 15.01.2007) --> observation needed --> value from CC is 0.43,, not confirmed by EtaCarinae (but doubtful obs) consistent with 1e0102 --> archive CAS should be check to available with different temperatures TASK 036: REPORT ON MOS ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Kirsch4.pdf -- 1052.9 Кб -- 13.05.2014 Похожие документы
... of MOS drm parameter files (SS) 15/2 Provide eff mode CTI degradation parameters to SOC Dennerl 15/3 15/4 * Implement modedept. pn CTIdegradation in SAS Kirsch/Saxton 20051019 20051019 NRCO on EtaCarinae in SW and FF mode, obs. time Kirsch like rev 115 ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200605/LMetcalfe.pdf -- 2728.8 Кб -- 14.05.2014 Похожие документы