  We present up-to-date metallicity-dependent temperature vs. color
calibrations for main sequence and giant stars based on temperatures derived
with the infrared flux method (IRFM). Seventeen colors in the following
photometric systems: UBV, uvby, Vilnius, Geneva, RI(Cousins), DDO,
Hipparcos-Tycho, and 2MASS, have been calibrated. The spectral types covered
range from F0 to K5 (7000 K<Teff<4000 K) with some relations extending below
4000 K or up to 8000 K. Most of the calibrations are valid in the metallicity
range -3.5<[Fe/H]<0.4, although some of them extend to as low as [Fe/H]=-4.0.
All fits to the data have been performed with more than 100 stars; standard
deviations range from 30 K to 120 K. Fits were carefully performed and
corrected to eliminate the small systematic errors introduced by the
calibration formulae. Tables of colors as a function of Teff and [Fe/H] are
provided. (Abridged)
