... stars

Based on observations collected at the European Southern Observatory, La Silla, Chile, Proposals #65.L-0019(B) and 67.B-0108(B).

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...

Full Tables 3 and 6 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/410/527

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...]

Abundances expressed within brackets are as usual relative to solar values where, for element X, $[X/{\rm H}]=\log (N_{X}/N_{\rm H})_{\star}-\log (N_{X}/N_{\rm H})_{\odot}$.

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... metallicities

Metallicities derived from photometry are denoted by " ${\rm [Me/H]}$''. Spectroscopic "metallicities'' are denoted by " $\rm [Fe/H]$'' and measure the iron content of the stars.

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...

The actual probabilities listed in Table 2 have been calculated using radial velocities that we determined from our FEROS spectra, see Sect. 4.

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... MIDAS

ESO-MIDAS is the acronym for the European Southern Observatory Munich Image Data Analysis System which is developed and maintained by the European Southern Observatory.

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... IRAF

IRAF is distributed by National Optical Astronomy Observatories, operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation, USA.

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