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Figure 16
(Left) Histograms of 100000 frames in the dark with different fine thresholds, for a single pixel. (Left inset) To centre the noise peak on approximately zero fine counts, the threshold at which 50% of frames give counts greater than zero is chosen, corresponding to a fine threshold of 1189. (Right) The means of the dark distribution for different fine thresholds (only those points shown in the residuals contributed to the linear fit).

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 33| Part 5| September 2026|
https://doi.org/10.1107/S1600577526006375
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