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The Swift Ultra-Violet/Optical Telescope
Authors:Peter W A Roming  Thomas E Kennedy  Keith O Mason  John A Nousek  Lindy Ahr  Richard E Bingham  Patrick S Broos  Mary J Carter  Barry K Hancock  Howard E Huckle  S D Hunsberger  Hajime Kawakami  Ronnie Killough  T Scott Koch  Michael K Mclelland  Kelly Smith  Philip J Smith  Juan Carlos Soto  Patricia T Boyd  Alice A Breeveld  Stephen T Holland  Mariya Ivanushkina  Michael S Pryzby  Martin D Still  Joseph Stock
Institution:(1) Department of Astronomy & Astrophysics, Pennsylvania State University, 525 Davey Lab, University Park, PA, 16802, U.S.A.;(2) Mullard Space Sciences Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, U.K.;(3) Southwest Research Institute, 6220 Culebra Rd, San Antonio, TX, 78228, U.S.A.;(4) Optical Science Laboratory, University College London, Gower St, London, WC1E 6BT, U.K.;(5) Starsys Research Corporation, 4909 Nautilus Court N., Boulder, CO, 80301, U.S.A.;(6) NASA/Goddard Space Flight Center, Code 660.1 Greenbelt, MD, 20771, U.S.A.;(7) Swales Aerospace, 5050 Powder Mill Rd, Beltsville, MD, 20705, U.S.A.;(8) Present address: Ball Aerospace, 1600 Commerce St, Boulder, CO, 80301, U.S.A.
Abstract:The Ultra-Violet/Optical Telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (∼1 min) UV and optical photons from the afterglow of gamma-ray bursts in the 170–600 nm band as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey–Chrétien design with micro-channel plate intensified charged-coupled device detectors that record the arrival time of individual photons and provide sub-arcsecond positioning of sources. We discuss some of the science to be pursued by the UVOT and the overall design of the instrument.
Keywords:Swift                  Ultra-Violet/Optical Telescope  gamma-ray burst  afterglow  spectroscopy  imaging
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