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Figure 2
k-range of EXAFS data recorded at ID24 using a DAC as a function of the working energy. In the energy range highlighted in purple (darker shading) the limitation is due to the large incident angle θ on the polychromator, while in the energy range highlighted in pale blue (lighter shading) it is due to the Bragg reflections from the diamonds.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 16| Part 6| September 2009| Pages 699-706
doi:10.1107/S0909049509037571
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