Fig. C.1
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Theoretical spectral resolving power of MISTRAL. The data for the blue and red configurations are from Table C.1. Top panel: Resolving power vs. wavelength. The straight lines are the linear fitting of these data. Bottom panel: FWHM vs. wavelength. The curves are computed from the linear fits. For comparison, the wavelength separation of several close stellar emission lines is marked with a diamond (resolved with MISTRAL) and crosses (unresolved with MISTRAL).
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