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Figure 3
(a) The fraction of X-rays incident on the detector resulting in absorbed energy for a 50 mm-thick layer of Gd2O2S as a function of photon energy. This is an approximation of the ideal detector's DQE. (b) Inverse of (a) and the DQE correction factor when determining the required number of incident X-rays.

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SYNCHROTRON
RADIATION
ISSN: 1600-5775
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