All Tables

• Table 1: 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 2: Photospheric lines identified in the FUSE spectrum. "*'' denotes lines with possibly inaccurately known wavelengths. ":'' denotes uncertain identifications.
• Table 3: Photospheric oxygen lines identified in the Chandra spectrum. ":'' denotes uncertain identifications. O V lines are not detectable ("-'') but included here, because their absence is discussed in the text.
• Table 4: Photospheric neon lines identified in the Chandra spectrum. ":'' denotes uncertain identifications.
• Table 5: Photospheric magnesium lines identified in the Chandra spectrum. ":'' denotes uncertain identifications. "bl'' denotes blends with lines of other elements.
• Table 6: Log of FUSE observations of H 1504+65.