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Título: | Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts |
Autor: | Jeong, S.; Nam, J.W.; Ahn, K.B.; Park, I. H.; Kim, S.W.; Lee, J.; Lim, H.; Brandt, S.; Budtz-Jørgensen, C.; Castro-Tirado, Alberto J. CSIC ORCID ; Chen, P.; Cho, M.H.; Choi, J.N.; Grossan, B.; Huang, M.A.; Jung, A.; Kim, J. E.; Kim, M. B.; Kim, Y.W.; Linder, E.V.; Min, K.W.; Na, G.W.; Panasyuk, M.I.; Ripa, J.; Reglero, V.; Smoot, G.F.; Suh, J.E.; Svertilov, S.; Vedenkin, N.; Yashin, I. | Palabras clave: | Light Mirrors Optical telescopes Stars Telescopes Gamma-ray bursts (GRBs) Gamma rays |
Fecha de publicación: | 2013 | Editor: | Optical Society of America | Citación: | Optics Express 21: 2263- 2278 (2013) | Resumen: | We report on design, manufacture, and testing of a Slewing Mirror Telescope (SMT), the first of its kind and a part of Ultra-Fast Flash Observatory-pathfinder (UFFO-p) for space-based prompt measurement of early UV/optical light curves from Gamma-Ray Bursts (GRBs). Using a fast slewing mirror of 150 mm diameter mounted on a 2 axis gimbal stage, SMT can deliver the images of GRB optical counterparts to the intensified CCD detector within 1.5∼1.8 s over ± 35 degrees in the slewing field of view. Its Ritchey-Chrétien telescope of 100 mm diameter provides a 17 × 17 arcmin2 instantaneous field of view. Technical details of design, construction, the laboratory performance tests in space environments for this unique SMT are described in conjunction with the plan for in-orbit operation onboard the Lomonosov satellite in 2013. © 2013 Optical Society of America. | Versión del editor: | http://dx.doi.org/10.1364/OE.21.002263 | URI: | http://hdl.handle.net/10261/133599 | DOI: | 10.1364/OE.21.002263 | Identificadores: | doi: 10.1364/OE.21.002263 issn: 1094-4087 |
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