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Figure 9
(a, b) Simulated XMCD data (thick solid lines) on a long and short delay range for the worst case scenario of [\beta] = 0.6. The thin solid lines represent the fits neglecting any halo contribution and a simplified halo contribution, respectively. (c, d) Initial magnetization dynamics m(t) and the results derived from the fits of the according upper panels (a) and (b). Note that panels (b) and (d) are not a zoom-in, instead the fit routines are applied only to the shown subset of the simulated slicing + halo XMCD data shown in (a).

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 23| Part 3| May 2016| Pages 700-711
doi:10.1107/S160057751600401X
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