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Fig. 3

image

Gaussian model for CIS of the star HD 149349 observed by the RAVE survey (R = 7500). Upper panel: black and blue lines show the observed and synthetic spectra, respectively. The atmospheric parameters from RAVE–DR6 are also indicated. Lower panel: renormalized interstellar spectrum represented by the black line. The dashed and solid red lines represent the profiles from the first and second (finally selected) fits, respectively. The blue shades indicate the masked regions discussed in Sect. 2.6.2.

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