Fig. 3
Model adjustment for Ogle N: 393009 (Teff = 5012 K). The DIB is in a region devoid of strong stellar lines. The upper panel shows the spectrum (red line) and the best-fit model (purple line). The lower panel shows the synthetic stellar model (yellow line), the synthetic atmospheric model (blue line), and the DIB profile (green line), which all correspond to the fit parameters.
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