We present optical spectra, obtained with the Keck 10 m telescope, of two h
igh-redshift Type Ia supernovae (SNe Ia) discovered by the High-z Supernova
Search Team: SN 1999ff at z = 0.455 and SN 1999fv at z similar to 1.2, the
highest redshift published SN Ia spectrum. Both SNe were at maximum light
when the spectra were taken. We compare our high-z spectra with low-z norma
l and peculiar SNe Ia as well as with SNe Ic, Ib, and II. There are no sign
ificant differences between SN 1999ff and normal SNe Ia at low redshift. SN
1999fv appears to be an SN Ia and does not resemble the most peculiar near
by SNe Ia.