Paper
23 October 1997 Focal planes and mount assemblies for the WIRE program
Bruce A. Beardwood, Charles Lynn Hern, David H. Seib, Maryn G. Stapelbroek, John C. Kemp
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Abstract
The wide-field infrared explorer (WIRE) is a small spaceborne cryogenic telescope specifically designed to study the evolution of starburst galaxies. The use of advanced, large format, infrared hybrid focal plane array technology provides a large sensitivity gain over previously flown missions. The hybrid focal plane arrays (HFPAs) used in this instrument are 128 by 128-element arsenic-doped-silicon blocked impurity band infrared detector arrays connected via indium column interconnects to matching cryogenic multiplexers. The WIRE instrument includes two focal plane mount assemblies (FPMAs), each of which includes a HFPA optimized for a particular wavelength band. Details concerning design, fabrication and performance of the critical components of the WIRE FPMAs are described.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bruce A. Beardwood, Charles Lynn Hern, David H. Seib, Maryn G. Stapelbroek, and John C. Kemp "Focal planes and mount assemblies for the WIRE program", Proc. SPIE 3122, Infrared Spaceborne Remote Sensing V, (23 October 1997); https://doi.org/10.1117/12.278998
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Cited by 1 scholarly publication.
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KEYWORDS
Beryllium

Sensors

Space telescopes

Satellites

Galactic astronomy

Multiplexers

Cryogenics

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