6 July 2018 Performance overview of the near infrared detectors in Korean space missions NISS and LIRS
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Abstract
NISS (Near-infrared Imaging Spectrometer for Star formation history) is a unique spaceborne imaging spectrometer (R = 20) onboard the Korea’s next micro-satellite NEXTSat-1 to investigate the star formation history of Universe in near infrared wavelength region (0.9 – 2.5 μm). In this paper, we introduce the NISS H2RG detector electronics, the test configuration, and the performance test results. Analyzed data will be presented on; system gain, dark current, readout noise, crosstalk, linearity, and persistence. Also, we present basic test results of a Korean manufactured IR detector, 640 x 512 InAsSb 15 μm pixel pitch, developed for future Korean lunar mission.
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Dae-Hee Lee, Dae-Hee Lee, Won-Kee Park, Won-Kee Park, Youngsik Park, Youngsik Park, Jeonghyun Pyo, Jeonghyun Pyo, Bongkon Moon, Bongkon Moon, Woong-Seob Jeong, Woong-Seob Jeong, Sung-Joon Park, Sung-Joon Park, Il-Joong Kim, Il-Joong Kim, Min-Gyu Kim, Min-Gyu Kim, Dukhang Lee, Dukhang Lee, Kyeong Yeon Ko, Kyeong Yeon Ko, Young-Jun Choi, Young-Jun Choi, Haingja Seo, Haingja Seo, SeungCheol Bang, SeungCheol Bang, Mihyun Kim, Mihyun Kim, Young-Ho Kim, Young-Ho Kim, Sung-Yong Ko, Sung-Yong Ko, Hyun-Jin Lee, Hyun-Jin Lee, } "Performance overview of the near infrared detectors in Korean space missions NISS and LIRS", Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 106984Q (6 July 2018); doi: 10.1117/12.2310056; https://doi.org/10.1117/12.2310056
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