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Ashley (UNSW), M. E. Ozel (Cag U.), N. Gehrels (NASA/Goddard), P. Schady (MSSL-UCL), P. T. O'Brien (U. Leicester), R. Filgas (MPE-Garching), R. M. Quimby (Caltech), R. Willingale (U. Leicester), S. B. Pandey (U. Mich), S. D. Barthelmy (NASA/Goddard), S. R. Oates (MSSL-UCL), T. A. McKay (U. Mich), T. Guver (U. Arizona), T. Kruhler (MPE-Garching), U. Kiziloglu (METU), W. Rujopakarn (U. Arizona), W. T. Vestrand (LANL), W. Zheng (U. Mich)","submitted_at":"2010-02-02T21:42:17Z","abstract_excerpt":"We present a multi-wavelength study of GRB 081008, at redshift 1.967, by Swift, ROTSE-III and GROND. Compared to other Swift GRBs, GRB 081008 has a typical gamma-ray isotropic equivalent energy output (10^53 erg) during the prompt phase, and displayed two temporally separated clusters of pulses. The early X-ray emission seen by the Swift/XRT was dominated by the softening tail of the prompt emission, producing multiple flares during and after the Swift/BAT detections. 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