  The Haystack 37-meter telescope was used in a pilot project in May 1995 to
observe GRB error boxes at 23~GHz. Seven BATSE error boxes and two IPN arcs
were scanned by driving the beam of the telescope rapidly across their area.
For the BATSE error boxes, the radio observations took place two to eighteen
days after the BATSE detection, and several boxes were observed more than once.
Total power data were recorded continuously as the telescope was driven at a
rate of 0.2~degrees/second, yielding Nyquist sampling of the beam with an
integration time of 50~milliseconds, corresponding to a theoretical rms
sensitivity of 0.5~Jy. Under conditions of good weather, this sensitivity was
achieved. In a preliminary analysis of the data we detect only two sources,
3C273 and 0552+398, both catalogued sources that are known to be variable at
23~GHz. Neither had a flux density that was unusally high or low at the time of
our observations.
