  The 2-m robotic Liverpool Telescope (LT) is ideally suited to the rapid
follow-up of unpredictable and transient events such as GRBs. Our GRB follow-up
strategy is designed to identify optical/IR counterparts in real time; it
involves the automatic triggering of initial observations, on receipt of an
alert from Gamma Ray Observatories HETE-2, INTEGRAL and Swift, followed by
automated data reduction, analysis, OT identification and subsequent observing
mode choice. The lack of human intervention in this process requires robustness
at all stages of the procedure. Here we describe the telescope, its
instrumentation and GRB pipeline.
