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Fig. 9
Comparison of spectra taken at two different phases (25 August 2018, ϕ = 0.08, shown as thesolid black line, and 29 September 2018, ϕ = 0.50, shown as the red dotted line) around selected lines. The vertical lines indicate the expected companion velocity for the orbital solution of Bjorkman et al. (2002).
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