I am posting from the APS meeting in Jacksonville.
You can see the preliminary result that was presented here,
with lots and lots of caveats,
by going to the GPb Homepage,
http://einstein.stanford.edu/index.html
and clicking on poster L1.00028,
Gravity Probe B Science Data Analysis: Filtering Strategy.
The result is called
"Glimpses of Frame Dragging"
and is in the bottom right quadrant of the poster.
One "glimpse" differs from GR by about two sigma,
but everything is still preliminary,
including the size of the sigma,
which is of order 10 mas/y
i.e. milliarcseconds per year.
I believe this particular "glimpse" is based on about 40 days data from one of the gyros.
Also, they have not yet unblinded themselves from the improved drift of the guidestar.
However, they still hope/expect to reduce their sigma to 1 or 2 mas/y by December.
Francis said there may be a small hint of a difference with GR,
but it is still much too early to talk about this seriously.
Jim Graber