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Figure 7
Probability distribution of measurable reflections in reciprocal space. A λ-curve of beamline ID09 with a wiggler W70/undulator U46 source at the ESRF is used. Darker grey levels indicate higher probability.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 6| Part 4| July 1999| Pages 891-917
doi:10.1107/S0909049599006366
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