Galaxy from the COSMOS survey with mBJ(estimated) =22.5; no CCD frames
taken. However the candidate is seen on PDS scanner plots of both the
ESO R and UKST IIIa-J plates and inspection of the IIIa-J plate
indicates a low-surface-brightness galaxy. Re-observed with VLA on
Apr 1995 and found to be a steep-spectrum source, thus excluding it
from our complete sample.