  The TeV emitting high-mass X-ray binary system LSI+61303 was observed with
the Swift satellite from early September 2006 to early January 2007. Many of
these observations were contemporaneous with TeV observations. The data consist
of observations on 24 separate days with durations ranging between 700s and
4700s, and partially cover 4.5 orbital periods of the binary system. We present
here an analysis of the 0.2 to 10keV X-ray data from the Swift-XRT instrument.
Contemporaneous optical data from UVOT are also available.
