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Various dedicated satellite projects are underway or in advanced stages ofplanning to perform high-precision, long duration time series photometry ofstars, with the purpose of using the frequencies of stellar oscillations to putnew constraints on the internal structure of stars. It is known (cf. Brown, etal. 1994) that the effectiveness of oscillation frequencies in constrainingstellar model parameters is significantly higher if classical parameters suchas effective temperature, and luminosity are known with high precision. Inorder to optimize asteroseismic campaigns it is therefore useful to selecttargets from among candidates for which good spectroscopic and astrometric dataalready exists. This paper presents selection criteria, as well asredeterminations of stellar luminosity and reddening for stars satisfying thesecriteria.Comment: 8 pages, LaTeX, aa.cls, txfonts.sty, graphicx.sty, to be published in  Astronomy & Astrophysic

Selection criteria for targets of asteroseismic campaigns