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Experiment of WFCT-II (Wide Field Cryogenic Telescope II) at Sutherland, South Africa

Published online by Cambridge University Press:  13 November 2008

K. Haraguchi*
Affiliation:
Dept. of Astrophysics, Nagoya University, 464-8602, Japan
S. Sato
Affiliation:
Dept. of Astrophysics, Nagoya University, 464-8602, Japan
M. Kurita
Affiliation:
Dept. of Astrophysics, Nagoya University, 464-8602, Japan
G. Weilai
Affiliation:
Dept. of Astrophysics, Nagoya University, 464-8602, Japan
T. Nagata
Affiliation:
Dept. of Astronomy, Kyoto University, 606-8502, Japan
T. Nagayama
Affiliation:
Dept. of Astronomy, Kyoto University, 606-8502, Japan
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Abstract

We have developed a Wide Field Cryogenic Telescope II (WFCT-II), which contains a whole telescope-optics in a cryostat to suppress thermal emission from the whole telescope. The cryostat is of a cylindrical shape of 800 mm length and 300 mm diameter. The telescope inside is a Ritchey-Chretien system with the primary mirror of 231 mm in diameter and a focal length of 1500 mm.
The InSb 1k × 1k infrared array detector (Aladdin II) has a FoV of 1 square degree and a resolution of 3'' × 3''/pixel.
We can install 5 filters whose wavelengths range from 1 μm to 5 μm.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2008

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References

Ando, M., et al., 2002, ApJ, 574, 187 CrossRef
Ando, M., et al., 2002, Exper. Astron., 13, 119 CrossRef