  Local and intermediate redshift (z~0.5) galaxy samples obey well correlated
relations between the stellar population luminosity and maximal galaxy rotation
that define the Tully-Fisher (TF) relation. Consensus is starting to be reached
on the TF relation at z~0.5, but work at significantly higher redshifts is even
more challenging, and has been limited by small galaxy sample sizes, the
intrinsic scatter of galaxy properties, and increasing observational
uncertainties. We present here the TF measurements of 41 galaxies at relatively
high redshift, spectroscopically observed with the Keck/DEIMOS instrument by
the DEEP2 project, a survey which will eventually offer a large galaxy sample
of the greatest depth and number yet achieved towards this purpose. The
'first-look' sample analyzed here has a redshift range of 0.75<z<1.3 with <z>=
0.85 and an intrinsic magnitude range from M_B of -22.66 to -20.57 (Vega). We
find that compared to local fiducial samples, a brightening of 1.5 magnitudes
is observed, and consistent with passive evolutionary models.
