The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 42 Issue 1
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- Pages.40.1-40.1
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- 2017
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- 1226-2692(pISSN)
Status Report of the Flight Model of the NISS onboard NEXTSat-1
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Jeong, Woong-Seob
(Korea Astronomy and Space Science Institute) ;
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Moon, Bongkon
(Korea Astronomy and Space Science Institute) ;
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Park, Sung-Joon
(Korea Astronomy and Space Science Institute) ;
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Lee, Dae-Hee
(Korea Astronomy and Space Science Institute) ;
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Pyo, Jeonghyun
(Korea Astronomy and Space Science Institute) ;
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Park, Won-Kee
(Korea Astronomy and Space Science Institute) ;
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Kim, Il-Joong
(Korea Astronomy and Space Science Institute) ;
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Park, Youngsik
(Korea Astronomy and Space Science Institute) ;
- Lee, Duk-Hang (Korea Astronomy and Space Science Institute) ;
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Ko, Kyeongyeon
(Korea Astronomy and Space Science Institute) ;
- Kim, Mingyu (Korea Astronomy and Space Science Institute) ;
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Nam, Ukwon
(Korea Astronomy and Space Science Institute) ;
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Kim, Minjin
(Korea Astronomy and Space Science Institute) ;
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Ko, Jongwan
(Korea Astronomy and Space Science Institute) ;
- Im, Myungshin (Seoul National University) ;
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Lee, Hyung Mok
(Seoul National University) ;
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Lee, Jeong-Eun
(Kyung Hee University) ;
- Shin, Goo-Hwan (Satellite Technology & Research Center, KAIST) ;
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Chae, Jangsoo
(Satellite Technology & Research Center, KAIST) ;
- Matsumoto, Toshio (Korea Astronomy and Space Science Institute)
- Published : 2017.04.10
Abstract
The NISS (Near-infrared Imaging Spectrometer for Star formation history) is the near-infrared spectro-photometric instrument optimized to the Next Generation of small satellite series (NEXTSat). To achieve the major scientific objectives for the study of the cosmic star formation in local and distant universe, the spectro-photometric survey covering more than 100 square degree will be performed. The main observational targets will be nearby galaxies, galaxy clusters, star-forming regions and low background regions. The off-axis optics was developed to cover a wide field of view (
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