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Fig. A.1.

Fig. A.1. Refer to the following caption and surrounding text.

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UVB X-shooter spectrum taken at phase 0.84 (gray) compared to our best-fitting TMAP models assuming a surface ratio of 0.17. Light gray regions indicate the location of a weak residual nebular and interstellar lines, which have been excluded from the fit. The red and blue lines represent the contribution of Star 1 and Star 2, respectively, and the dashed, purple line shows the combined fit.

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