Fig. B.1.
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Best-fit NLTE model (red) to the spectrum of the PG 1159-type central star of BMP J0739-1418 (blue). The significant lines due to principal ions in the model are identified, as are the location of calcium and sodium interstellar lines (i.s.), a diffuse interstellar band (DIB), and telluric absorption. The model atmosphere parameters are shown in Table 2.
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