Fig. B.2.
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Modelling of the C III] line profile for the spectra taken by the NOT and TNG telescopes. Top left: TNG spectrum from May 28 (first exposure). Top middle: TNG spectrum from May 28 (second exposure). Top right: NOT spectrum from June 18. Bottom left: TNG spectrum from July 3 (first exposure). Bottom right: TNG spectrum from July 3 (second exposure). The spectra are fitted with one Gaussian component plus a linear function. The total fitted model is represented in black. The bottom panels show the residuals of the fits.
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