Bulletin of the Korean Space Science Society (한국우주과학회:학술대회논문집(한국우주과학회보))
- 2011.04a
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- Pages.23.1-23.1
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- 2011
Performance Measurement of SMT(Slewing Mirror Telescope) Optical System
- Ahn, Ki-Beom (Space Optics Laboratory, Dept. of Astronomy, Yonsei University) ;
- Jeong, Soo-Min (Research Center of the MEMS Space Telescope, Dept. of Physics, Ewha Womans University) ;
- Kim, Ji-Eun (Research Center of the MEMS Space Telescope, Dept. of Physics, Ewha Womans University) ;
- Kim, Sug-Whan (Space Optics Laboratory, Dept. of Astronomy, Yonsei University) ;
- Lee, Jik (Research Center of the MEMS Space Telescope, Dept. of Physics, Ewha Womans University) ;
- Lim, Heui-Jin (Institute for the Early Universe, Ewha Womans University) ;
- Lindere, V. (Institute for the Early Universe, Ewha Womans University) ;
- Nam, Ji-Woo (Research Institute for Basic Sciences, Ewha Womans University) ;
- Nam, Koo-Hyun (Research Center of the MEMS Space Telescope, Dept. of Physics, Ewha Womans University) ;
- Park, Il-H. (Research Center of the MEMS Space Telescope, Dept. of Physics, Ewha Womans University) ;
- Smoot, G.F. (Institute for the Early Universe, Ewha Womans University)
- Published : 2011.04.15
Abstract
The SMT is a subsystem of the UFFO (Ultra-Fast Flash Observatory) pathfinder onboard the Lomonosov spacecraft planed to be launched in November 2011. The UFFO is designed for extremely fast observation of optical afterglow of Gamma Ray Burst (GRB). This study is primarily concerned with performance measurement of the SMT optical system under the integration and test phase. SMT is a 100mm Ritchey-Chretien type telescope with a motorized slewing mirror and a
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