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Real-time algorithms for optimal CCD data reduction in high energy astronomy

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Figure

Figure 1.1: Arrangem ent of mirrors, gratings and CCDs in the RGS. X-rays arrive at the top
Figure 1.3: Plot of resolving power vs. photon energy showing the figures necessary to perform
Figure lA : Effective area of the XM M -N ew ton mirrors plotted as a function of energy, and shown
Figure 1.5: N et effective area of the mirrors when folded in with the responses of the individual instru­
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