  We present spectroscopy of 285 previously identified candidate members of
populations in the Sco-Cen complex, primarily Ophiuchus, Upper Sco, and Lupus.
The spectra are used to measure spectral types and diagnostics of youth. We
find that 269 candidates exhibit signatures of youth in our spectra or previous
data, which is consistent with their membership in Sco-Cen. We have constructed
compilations of candidate members of Ophiuchus, Upper Sco, and Lupus that have
spectral classifications and evidence of youth, which contain a total of 2274
objects. In addition, we have used spectra from previous studies to classify
three sources in Ophiuchus that have been proposed to be protostellar brown
dwarfs: ISO Oph 70, 200, and 203. We measure spectral types of early M from
those data, which are earlier than expected for young brown dwarfs based on
evolutionary models (>=M6.5) and instead are indicative of stellar masses (~0.6
Msun).
