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Table 1

Spectra used for the analysis.

Star Instrument Range (Å) R S/N
HD 127493 IUE SWP 1150–1970 10 000 14
GHRS 1225–1745 0.07 Å (a) 40
IUE LWR 1850–3273 10 000 14
FEROS 3700–9200 48 000 180
HZ 44 FUSE 905–1188 19 000 30
IUE SWP 1150–1970 10 000 10
HIRES 3022–7580 36 000 142
ISIS 3700–5260 1.5 Å(a) 170

Notes. The signal-to-noise ratio is the average over the spectrum. (a) The resolution for long-slit spectrographs is given instead as Δλ.

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