Several large scale photometric and spectroscopic surveys are being undertaken to provide a more detailed picture of the Milky Way. Given the necessity of generalisation in the determination of, e.g., stellar parameters when tens and hundred of thousands of stars are considered it remains important to provide independent, detailed studies to verify the methods used in the surveys.
Cone search capability for table J/A+A/521/A40/table2 (Dwarf stars with both Stroemgren photometry and [Fe/H] based on high resolution, high S/N spectroscopy)