  We present a new timing solution for PSR B1534+12, based on
coherently-dedispersed observations at Jodrell Bank and, recently, Arecibo. The
new data have resulted in improved measurements of the post-Keplerian timing
parameters, including the orbital period derivative. At present, the
poorly-known distance to the pulsar limits the precision of the measurement of
the intrinsic orbital period derivative, and hence the strength of the test of
general relativity that results from this binary system. By assuming that
general relativity is the correct theory of gravity, we may invert the test and
find an improved value of the pulsar distance.
