  Based on CHARA Array measurements, we present the angular diameters of 23
nearby, main- sequence stars, ranging from spectral type A7 to K0, five of
which are exoplanet host stars. We derive linear radii, effective temperatures,
and absolute luminosities of the stars using HIPPARCOS parallaxes and measured
bolometric fluxes. The new data are combined with previously published values
to create an Angular Diameter Anthology of measured angular diameters to
main-sequence stars (luminosity class V and IV). This compilation consists of
125 stars with diameter uncertainties of less than 5%, ranging in spectral
types from A to M. The large quantity of empirical data are used to derive
color-temperature relations to an assortment of color indices in the Johnson
(BVRIJHK), Cousins (RI), Kron (RI), Sloan (griz), and WISE (W3W4) photometric
systems. These relations have an average standard deviation of ~3% and are
valid for stars with spectral types A0 to M4. To derive even more accurate
relations for Sun-like stars, we also determined these temperature relations
omitting early-type stars (Teff > 6750 K) that may have biased luminosity
estimates because of rapid rotation; for this subset the dispersion is only
~2.5%. We find effective temperatures in agreement within a couple percent for
the interferometrically characterized sample of main sequence stars compared to
those derived via the infrared-flux method and spectroscopic analysis.
