19 January 1984 Cryogenic Telescope On The Infrared Astronomical Satellite (IRAS)
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Proceedings Volume 0430, Infrared Technology IX; (1984); doi: 10.1117/12.936400
Event: 27th Annual Technical Symposium, 1983, San Diego, United States
Abstract
The Infrared Astronomical Satellite (IRAS) has completed an unbiased all-sky survey at wavelengths from 10 to 100 um. The design and performance of the focal plane array is described with emphasis on in-orbit measurements of the sensitivity and stability. In the four broad spectral bands centered at 12, 25, 60 and 100 um the system NEFD values are, in Jy/Hz1/2,0.03, 0.025, 0.046 and 0.21 respectively (Jansky = 1E-26 w/m2/Hz). For point sources, a single scan at the survey rate of 3.8 arcmin/sec yields limiting flux densities at the 3 sigma confidence level of 0.36 , 0.30, 0.39 and 1.2 Jy. The DC stability of the JFET amplifiers and the excellent off-axis rejection of the telescope permit total flux meaurements of extended infrared emission at levels below 1 E 6 Jy/sr. Response of the extrinsic silicon and germanium photodetectors to ionizing radiation is described.
© (1984) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
F. J. Low, C. A. Beichman, F. C. Gillett, J. R. Houck, G. Neugebauer, D. E. Langford, R. G. Walker, R. H. White, "Cryogenic Telescope On The Infrared Astronomical Satellite (IRAS)", Proc. SPIE 0430, Infrared Technology IX, (19 January 1984); doi: 10.1117/12.936400; https://doi.org/10.1117/12.936400
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KEYWORDS
Sensors

Infrared radiation

Field effect transistors

Telescopes

Infrared sensors

Infrared telescopes

Infrared detectors

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