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Figure 19
Results from modified SeAFFluX after rescaling and averaging over pixels. From top to bottom: 10 K, 50 K, 100 K, 150 K. The fine structure of the XAFS (right) matches perfectly with small overarching deviations due to the spline fitting. The noise is visibly larger in the fluorescence spectra than in transmission, but all the detail of the XAFS is clearly visible. With careful analysis, just as much structure can be seen in fluorescence analysis as in transmission.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 30| Part 1| January 2023| Pages 147-168
https://doi.org/10.1107/S1600577522010293
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