21 October 1996 Flight performance of the Near-Infrared Spectrometer
Author Affiliations +
Abstract
The near-infrared spectrometer (NIRS) is one of the focal plane instruments of the infrared telescope in space (IRTS). The NIRS is a simple grating spectrometer with two element InSb linear arrays, and was designed to measure the absolute sky brightness at the wavelengths from 1.4 to 4.0 micrometer with a spectral resolution of 0.13 micrometer and a beam size of 8 feet by 8 feet. The IRTS was launched on 1995 March 18. The NIRS worked well throughout the observation period from March 29 to April 25, and scanned about 7% of the entire sky. Multiple passage of bright stars through the NIRS field of view enabled us to reconstruct the beam pattern and to calibrate the sensitivity. Those flight data confirmed good performance of the NIRS on the orbit as was expected from the preflight measurements.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Manabu Noda, Manabu Noda, Toshio Matsumoto, Toshio Matsumoto, Hiroshi Murakami, Hiroshi Murakami, Mitsunobu Kawada, Mitsunobu Kawada, Masahiro Tanaka, Masahiro Tanaka, Shuji Matsuura, Shuji Matsuura, Hongfeng Guo, Hongfeng Guo, } "Flight performance of the Near-Infrared Spectrometer", Proc. SPIE 2817, Infrared Spaceborne Remote Sensing IV, (21 October 1996); doi: 10.1117/12.255185; https://doi.org/10.1117/12.255185
PROCEEDINGS
10 PAGES


SHARE
RELATED CONTENT


Back to Top