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Figure 4
Angular dependence of the Gd L3 edge XMCD amplitude (filled circles) obtained by field flipping The data are fitted to the modeled circular polarization, P[^{\,\prime}_{\rm C}], which is given by (4)[link] (full line) and is convoluted with a Gaussian function of 15 arcsec FWHM. Note that for this experiment the beam size was larger than in §3[link], and therefore the beam divergence is increased.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
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