Volume 525, January 2011
|Number of page(s)||12|
|Section||Galactic structure, stellar clusters and populations|
|Published online||07 December 2010|
The following table reports the line list and atomic parameters adopted for Pal1-I and the Sun. For the Mn and Co lines we adopted the HFS of Prochaska et al. (2000). The measured equivalent width and the corresponding abundance obtained for each line are also reported.
Adopted line list and atomic parameters. The measured equivalent width and the corresponding abundances obtained for each line are also reported for both Pal1-I and the Sun.
© ESO, 2010
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