  We report an SMA interferometric identification of a bright submillimeter
source, GOODS 850-5. This source is one of the brightest 850 um sources in the
GOODS-N but is extremely faint at all other wavelengths. It is not detected in
the GOODS HST ACS images and only shows a weak 2 sigma signal at 1.4 GHz. It is
detected in the Spitzer IRAC bands and the MIPS 24 um band, however, with very
low fluxes. We present evidence in the radio, submillimeter, mid-IR, near-IR,
and optical that suggest GOODS 850-5 may be a z>4 galaxy.
