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Figure 5
(Top) Distribution of the standard deviation of dark noise, which is averaged over dark images. Closed and open symbols correspond to the results for the CCD and CMOS, respectively (circles: without binning; triangles: 2×2 binning; squares: 3×3 binning). To compare the different configurations, both abscissas and ordinates are normalized. The abscissas are normalized by the number of pixels in a bin. The ordinates are normalized by the number of pixels in a single frame. (Bottom) Semi-log plot of the result for the CCD without binning. The solid line indicates the fitting result with a Gaussian function.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 17| Part 6| October 2010| Pages 737-742
doi:10.1107/S090904951003726X
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