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.
Performance overview of the near infrared detectors in Korean space missions NISS and LIRS
Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave ; 2018 ; Austin,Texas,United States
Proc. SPIE ; 10698
2018-07-06
Conference paper
Electronic Resource
English
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