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Figure 5
Ratio of a few spectra normalized by the incident charge and corrected for dead-time losses in the SMPf framework, to the spectrum acquired at the lowest rate, also normalized by the charge, equation (23)[link]. The spectra were compressed, and each bin corresponds to 210 eV. (a) ML spectra and (b) L spectra.

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SYNCHROTRON
RADIATION
ISSN: 1600-5775
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