Fig. 3
Comparison of the best-fit CoMBiSpeC model (dots) with the ESPaDOns spectra of Spica at orbital phases 0.152 (15 March) and 0.841 (26 March; shifted by +0.2 continuum units). The tracing shown at the bottom is the difference between the 15 March spectrum and its corresponding synthetic spectrum and shows that the fit is good to ~3%.
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