We present optical identifications and redshifts for 17 new hi,oh-redshift
radio sources. Fifteen of these sources are radio galaxies; the remaining t
wo are high-redshift, steep-spectrum, radio-loud quasars. These objects wer
e discovered as part of an ongoing study of compact (theta < 10 "), moderat
ely steep spectrum (alpha(1.4 GHz)(4.8 GHz) > 0.75, S-v proportional to v(-
alpha)) sources from the MIT-Green Bank (MG) radio catalog (S-5 (GHz) great
er than or similar to 50 mJy). Spectra for the optical counterparts were ob
tained at the W. M. Keck Telescopes and are among the optically faintest ra
dio galaxies thus far identified. Redshifts range between 0.3 and 3.6, with
13 of the 17 at redshifts greater than 1.5. Combining these new radio gala
xies with two published MG radio galaxy spectra, we synthesize a composite
MG radio galaxy spectrum and discuss the properties of these galaxies in co
mparison with other, more powerful, radio galaxies at similar redshifts. We
suggest a radio power-ionization state relation.