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Figure 4
(a) Reconstruction r.m.s. error in real space, averaged over many independent reconstructions, as a function of counting time. The solid line shows the best fit to the data points by a power law. (b) Distribution of the r.m.s. error in two sets of independent reconstructions for counting times of 10 s and 1 s.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
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