EDP Sciences
Free Access
Issue
A&A
Volume 496, Number 3, March IV 2009
Page(s) 701 - 712
Section Galactic structure, stellar clusters, and populations
DOI https://doi.org/10.1051/0004-6361/200811070
Published online 09 February 2009

Online Material

Table 7:   Line list of our 816 metal lines in the wavelength range observed. The seven columns give (1) the wavelength in air; (2) the excitation energy of the lower level; (3) $\log gf$; (4) the radiation damping parameter (when no value was available the very low value of 1.00 $\times $ 105 was used); (5) the van der Waals damping marked with an ``A'' when calculated according to Anstee & O'Mara (1995), Barklem et al. (2000) and references therein, Barklem & Aspelund-Johansson (2005), or Barklem P., private communication (if a number is instead given this is an empirical correction factor to the van der Waals damping computed according to Unsöld (1955)); (6) the atomic or ionic species; and (7) a star ``*'' when the $\log gf$ value has been modified by spectrum fits to the spectra of th Sun and Arcturus.


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