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Figure 11
(a) The energy spectrum after CSA (black line) and after the proposed correction technique (red line) with the fitting function of Fig. 11[link](b). (b) 2D scatter plot of the energy ECSA of the coincidence events (m = 2), between pixels 5 and 6, after CSA. The energy ECSA is plotted versus the charge-sharing ratio R, which gives information about the interaction position of the events. The red line represents the best-fitting function used to correct charge losses after CSA.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
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