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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 10/2017, Volume 606, p. A94
.... We derive chemical abundances of Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd and Eu for a large sample of more than 1000 FGK dwarf stars with high-resolution ($R \sim$\,115000... 
Galaxy: Disk | Galaxy: Evolution | Stars: Abundances | Stars: Fundamental parameters | Solar neighborhood
Journal Article
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Publications of the Astronomical Society of Japan, ISSN 0004-6264, 10/2008, Volume 60, Issue 5, pp. 1159 - 1171
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