A research group led by Prof. WANG Jian from the University of Science and Technology of China (USTC) of the Chinese Academy of Sciences (CAS) proposed a continuous-scanning near-infrared sky brightness monitor (CNISBM). It can measure 2.5 to 5 um infrared sky brightness based on an InSb detector and a linear variable filter. This study was published on Jouranl of Astronomical Telescopes,
Monday, August 31, 2020
USTC researchers design continuous-scanning sky brightness monitor in 2.5- to 5-um band
Hefei, China (SPX) Sep 01, 2020
A research group led by Prof. WANG Jian from the University of Science and Technology of China (USTC) of the Chinese Academy of Sciences (CAS) proposed a continuous-scanning near-infrared sky brightness monitor (CNISBM). It can measure 2.5 to 5 um infrared sky brightness based on an InSb detector and a linear variable filter. This study was published on Jouranl of Astronomical Telescopes,
A research group led by Prof. WANG Jian from the University of Science and Technology of China (USTC) of the Chinese Academy of Sciences (CAS) proposed a continuous-scanning near-infrared sky brightness monitor (CNISBM). It can measure 2.5 to 5 um infrared sky brightness based on an InSb detector and a linear variable filter. This study was published on Jouranl of Astronomical Telescopes,
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