  A list of 50 bright Detached Eclipsing Binaries proposed for precise parallax
measurements for the FAME is presented. The eclipsing binaries, with precise
distances and with photometric and double-line spectroscopic orbits determined,
are essential for a full calibration of relations that could be used for very
precise distance determination of globular clusters, LMC, SMC, and perhaps also
M31 and M33.
