  Between September 2006 and February 2007, the galactic binary LS I +61 303
was monitored in the TeV band with the VERITAS array of imaging Cherenkov
telescopes. These observations confirm LS I +61 303 as a variable TeV gamma-ray
source, with emission peaking between orbital phase 0.6 and 0.7. During this
observational period, monitoring in the X-ray regime was also carried out using
both the RXTE and Swift detectors, which offered complementary coverage of the
source. Outbursts in the 0.2-10 keV band were observed by both satellites at
close to the same orbital phase as the TeV peak during the 2 orbital cycles
covered simultaneously in both bands. While this source has been extensively
studied in the X-ray band in the past, this is the first observational campaign
to utilize contemporaneous X-ray and TeV data on LS I +61 303.
