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31 March 1982 Development And Evaluation Of Integrated Infrared Arrays For Astronomical Applications
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The status of a technology program to evaluate existing infrared detector arrays and to develop improved ones for low-background astronomical applications is described. For applications such as the Shuttle Infrared Telescope Facility (SIRTF), arrays that cover as much of the 1-1000 μm range as possible are of interest. Low-background test results for 2 x 64 Si:Bi charge-injection-device and 1 x 20 InSb charge-coupled-device arrays are included. As a result of our testing, we plan to develop improved, astronomy-optimized extrinsic silicon arrays in both linear and area formats. Efforts to develop accumulation-mode MOSFETs specifically for liquid helium temperatures, and cryogenic amplifier and multi-plexer circuits, are discussed.
© (1982) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Craig R. McCreight "Development And Evaluation Of Integrated Infrared Arrays For Astronomical Applications", Proc. SPIE 0304, Modern Utilization of Infrared Technology VII, (31 March 1982);


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