  The Faulkes Telescope Project is an educational and research arm of the Las
Cumbres Observatory Global Telescope Network (LCOGTN). It has two 2-metre
robotic telescopes, located at Haleakala on Maui (FT North) and Siding Spring
in Australia (FT South). It is planned for these telescopes to be complemented
by a research network of eighteen 1-metre telescopes, along with an educational
network of twenty-eight 0.4-metre telescopes, providing 24 hour coverage of
both northern and southern hemispheres.
  We have been conducting a monitoring project of 13 low-mass X-ray binaries
(LMXBs) using FT North since early 2006. The introduction of FT South has
allowed us to extend this to monitor a total of 30 LMXBs. New instrumentation
will allow us to expand this project to include both infrared wavelengths (z
and y band) and spectroscopy. Brighter targets (~ 16 - 18 mag.) are imaged
weekly in V, R and i' band (SNR ~ 50), while fainter ones (> 18 mag.) are
observed only in i' band (SNR ~ 20). We alter this cadence in response to our
own analysis or Astronomers Telegrams (ATels).
