We report the epitaxial growth of GaSb using trimethylgallium (TMGa) o
r triethylgallium (TEGa) with trimethylantimony (TMSb), triethylantimo
ny (TESb), or trisdimethylaminoantimony (TDMASb) in a low-pressure ver
tical rotating-disk reactor. Growth is kinetically limited for TMGa in
the temperature range 560 to 640 degrees C, and is mass-transport lim
ited for TEGa in the range 525 to 640 degrees C. A minimum V/III ratio
is necessary to obtain stoichiometric GaSb, and is dependent on the p
yrolysis temperature of Ga and Sb precursors. Featureless morphology i
s achieved for layers grown with TMGa or TEGa and TMSb, while surface
defects are observed for layers grown with TEGa and TESb or TDMASb. Th
ese observations are consistent with Fourier transform infrared measur
ements, which indicate interactions between TEGa and TESb or TDMASb. A
ll nominally undoped layers are p-type, with overall superior properti
es being obtained for layers grown with TEGa and TMSb. However, growth
conditions that yield layers with the best electrical properties do n
ot necessarily correspond to the same conditions for highest optical q
uality.