Yost, S. A.Rykoff, E. S.Aharonian, F.Akerlof, C. W.Ashley, M. C. B.Barthelmy, S.Gehrels, N.2025-01-272025-01-2720060-7354-0326-00094-243Xhttps://hdl.handle.net/20.500.12428/2782916th Annual Astrophysics Conference -- NOV 29-DEC 02, 2005 -- Washington, DCWe report the successful performance of the Robotic Optical Transient Search Experiment (ROTSE) to promptly-disseminated Swift GRB triggers. ROTSE-III is a worldwide network of 4 unfiltered 0.45m optical telescopes. The telescopes operate robotically, automatically responding to GRB position triggers with a preset observations sequence. Including weather and other downtime, ROTSE-III can immediately respond to similar to 40% of Swift trigger positions, with shutter open within approximately 6-8 seconds from the trigger dissemination. We discuss improvements made possible in the automated response the the small, accurate Swift error boxes. We report ROTSE-III's general results, including OTs discovered or confirmed, the distribution of imaging start times relative to the GRB duration, and an overview of OT lightcurves.eninfo:eu-repo/semantics/closedAccessgamma-raysburst optical instrumentsROITSE-III performance in the swift eraConference Object836349+N/AWOS:000238125000069