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The 2-m robotic Liverpool Telescope (LT) is ideally suited to the rapidfollow-up of unpredictable and transient events such as GRBs. Our GRB follow-upstrategy is designed to identify optical/IR counterparts in real time; itinvolves the automatic triggering of initial observations, on receipt of analert from Gamma Ray Observatories HETE-2, INTEGRAL and Swift, followed byautomated data reduction, analysis, OT identification and subsequent observingmode choice. The lack of human intervention in this process requires robustnessat all stages of the procedure. Here we describe the telescope, itsinstrumentation and GRB pipeline.Comment: 4 pages, 1 figure, submitted to Il nuovo cimento (4th Workshop  Gamma-Ray Bursts in the Afterglow Era, Rome, 18-22 October 2004

The Liverpool Telescope Automatic Pipeline for Real-time GRB Afterglow Detection