Analytic study of grid star and reference star selection for the Space Interferometry Mission

Grid stars and reference stars provide the fundamental global and local astrometric reference frames for observations by the Space Interferometry Mission. They must therefore be astrometrically stable at the similar to1 mu as level. I present simple formulae in closed form to estimate the contamination of these frames by motions due to stellar companions that go undetected in a radial-velocity (RV) survey of specified precision. The contamination rate depends almost entirely on the binary-period distribution function and not on the details of the mass or eccentricity distributions. Screening by a modest RV survey (sigma (RV) = 60 m s(-1)) can reduce the fraction of grid stars with detectable unmodeled accelerations to much less than 1%. Reference-star selection promises to be much more challenging, partly because the requirements of astrometric stability are more severe and partly because the required density of sources is similar to 100 times higher, the latter of which implies that less satisfactory candidates will have to be accepted. The tools presented here can help design a reference-star selection strategy, but a full treatment of the problem will require better knowledge of their companions in the planetary mass range.