Like Fig. A.1, but for the PG1159 star GSC 08265. Overplotted is the final model (red) with T_eff = 72 000 K, log g = 4.8, and element abundances as given in Table 2. Red identification labels indicate lines that are not included in the model. Note the presence of highly excited C IV lines at locations indicated by horizontal blue and green bars (with principal quantum numbers marked). They are not included in the model except for the 7 → 10 transitions at 5470 Å. Question marks indicate unidentified photospheric lines.