... The nonflatness by itself produces a size of 106 Їm; all perturbations other than the telescope together pro duce 181 Їm. I used the 'equivalent Gaussian' distribution plotted in Figure 1, to calculate the ef fect of the flatter substrates. ...
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... S c o n t a m in a t io n h is t o r y 2010 EPIC BOC 23 March 2010 R G S r e c t if ic a t io n f o r X MM U G · XCal SAS v9.0.0 sample of 106/148 spectra and models · 3 C 2 7 3 , P K S 2 1 5 5 -3 0 4 , H 1 4 2 6 + 4 2 8 , P K S 0 5 4 8 -3 2 2 , M k n 5 ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201003/pollock-AMTP-RGS.pdf -- 228.2 Кб -- 13.05.2014 Похожие документы
... MPE Garching XMM-Newton EPIC Calibration Meeting, Mallorca, Spain, 01 Feb 2005 1 06 05 04 01 02 03 m g 0| l g r {z g % %h H y ykgq ei h g h% p g h f x w vq v jvu vi Rt h sr Hg 8f h gd m ge l j j W 8f h qp m y &q ed x f w p vu t sf v g r q p h g %i oh n 8i ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/mf_fastshiftcti.pdf -- 957.9 Кб -- 16.05.2014 Похожие документы
... Fordham, J. L. A., Bone, D. A., Oldfield, M. K., Bellis, J. G., Norton, T. J. The MIC photon counting detector, Proceedings of an ESA Symposium on Photon Detectors for Space Instrumentation p 103-106 (1994). ...