DEVELOPMENT OF SLEWING MIRROR TELESCOPE OPTICAL SYSTEM FOR THE UFFO-PATHFINDER

被引：0
|
作者：
Jeong, S. [1 ]
Nam, J. W.
Ahn, K. -B.
Park, I. H.
Kim, S. -W.
Lee, J.
Lim, H.
Brandt, S.
Budtz-Jorgensen, C.
Castro-Tirado, A. J.
Chen, P.
Cho, M. H. [1 ]
Choi, J. N.
Grossan, B.
Huang, M. A.
Jung, A. [1 ]
Kim, J. E. [1 ]
Kim, M. B.
Kim, Y. W. [1 ]
Linder, E. V.
Min, K. W.
Na, G. W. [1 ]
Panasyuk, M. I.
Ripa, J.
Reglero, V.
Smoot, G. F.
Suh, J. E. [1 ]
Svertilov, S.
Vedenkin, N.
Yashin, I.
机构：
[1] Ewha Womans Univ, Dept Phys, Seoul 120750, South Korea
来源：
GAMMA-RAY BURSTS: 15 YEARS OF GRB AFTERGLOWS - PROGENITORS, ENVIRONMENTS AND HOST GALAXIES FROM THE NEARBY TO THE EARLY UNIVERSE | 2013年 / 61卷
关键词：
D O I：
10.1051/eas/1361090
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chretien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 x 17 arcmin(2) in Field of View and 4.3 arcsec resolution (full width half maximum of the point spread function) The beam-steering mirror enables the SMT to access a 35 x 35 degree region and point and settle within 1 sec. All mirrors were fabricated to about 0.02 wavelengths RMS in wave front error (WFE) and 84.7% average reflectivity over 200 nm similar to 650 nm. The RC telescope was aligned to 0.05 wavelengths RMS in WFE (test wavelength 632.8 nm). In this paper, the technical details of the RC telescope and slewing mirror system assembly, integration, and testing are given shortly, and performance tests of the full SMT optical system are reported.
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收藏
页码：561 / 565
页数：5
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