Fig. C.2
A comparison of three individual Ondřejov spectra of HD 32328 (black lines) having the highest S/N with the model spectra (red lines). From top to bottom, the spectra were taken on RJD 56 011.4508, 56 013.4003, and 56 015.2794, respectively. Note that we could not remove the telluric lines from the observed spectra in this case.
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