Table 8: Lines used to derive the solar Os abundance. Abundances are derived using either the Holweger-Müller or MARCS models.
Wavelength $\log gf$* $\log \varepsilon_{\rm Os}$
(nm)   H - M MARCS
       
326.7945 -1.09 1.40 1.30
330.1559 -0.74 1.30 1.25
442.0468 -1.20 1.15 1.10


Average   1.28 1.22
Global average   1.25


* Deduced from semi-empirical gA-values of Table 5. Uncertainties are estimated to be about 20-25%.


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