  Astrophysical jets seem to gain strength disproportionate to the power of
their associated accretion flow, making low-luminosity sources ideal targets
for studies of the role of outflows. Radio/X-ray correlations have supported
the case for a strong relationship between the jets and the hard X-ray emitting
regions, and here we explore the strongest scenario where the base of the jets
subsumes the role of the corona. The properties of coronae, as inferred from
spectral models, are very similar to what is empirically required at jet bases
assuming conservation laws hold. We present a few preliminary fits to
simultaneous radio and X-ray data sets from our GX 339-4 and Cyg X-1 campaigns.
The fits are performed in detector space, and include a jet plus thermal disk
continuum model, with added Gaussian line and non-relativistic reflection
features similar to the approach of other X-ray models. We find that we can fit
the entire radio through X-ray spectrum quite well, with any deviation
occurring in the line/reflection region. The results suggest that a jet/corona
unification can provide a reasonable description of the data. Future work will
benefit from a more complex approach to the disk feedback features.
