Fig. 18.
Left: BP simulated spectrum with GOG (Luri et al. 2014) for a WC Wolf-Rayet star (HD 32257). Right: relative residuals obtained for the predicted epoch observation in CCD number 7. We note that, in BP, the wavelength decreases when the pseudo-wavelength increases, and values smaller than 15 fall outside the nominal range of the instrument (with λ > 680 nm), as can be seen in Fig. 4.
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