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Figure 1
Calculated brilliance generated by the SCW source of the XDS beamline (blue). The brilliance of the standard 1.67 T bending dipoles is also shown (red). Note the increase in brilliance, in particular at energies above 10 keV.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 23| Part 6| November 2016| Pages 1538-1549
https://doi.org/10.1107/S160057751601403X
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