All Tables

• Table 1: Identified photospheric lines (rest wavelengths) in the FUSE spectrum of PG 1159-035.
• Table 2: Photospheric lines (rest wavelengths) in the HST spectrum.
• Table 3: Radial-velocity shift of selected photospheric lines.
• Table 4: Unidentified photospheric lines in the FUSE and HST spectra (rest wavelengths). We remark whether the lines are detectable in high-resolution spectra of other PG 1159 stars or H-rich central stars as well.
• Table 5: Summary of the model atoms used in the model atmosphere and line formation calculations. The numbers in brackets give the individual line numbers summed into superlines for the heavy metal ions.
• Table 6: Newly determined positions of O VI lines as used in our improved model atom. We compare them to the literature values. The measurements were made in the PG 1159-035 spectra described in this paper (J06) as well as in spectra of other PG 1159 stars (Reiff et al. 2006, R06) and hot central stars (Traulsen et al. 2005, T05).
• Table 7: Photospheric and stellar parameters of PG 1159-035. We list the direct results from spectroscopic analyses and derived quantities (mass, luminosity, distance) from comparison with evolutionary tracks. Elemental abundances are given in mass fractions (2nd column) and relative to solar abundances (Grevesse & Sauval 2001 values;3rd column).