We present H and K spectra (showing redshifted H alpha, H beta and [O
III] emission lines) of three radio-loud and three radio-quiet quasars
with redshifts z greater than or similar to 2, which were obtained us
ing CGS4 on UKIRT. The [O III] lambda lambda 4959 + 5007 lines are too
weak to allow accurate determination of the redshift of the forbidden
lines. The observed Balmer decrements are consistent with enhancement
of H alpha due to collisional excitation.