Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1130..166w&link_type=abstract
IN: New technologies for astronomy; Proceedings of the Meeting, Paris, France, Apr. 25, 26, 1989 (A90-37976 16-89). Bellingham,
Astronomy and Astrophysics
Astronomy
Infrared Astronomy, Infrared Detectors, Systems Engineering, Design Analysis, Functional Design Specifications
Scientific paper
An evaluation is made of currently available IR detector arrays, with a view to devices under development which will become available in the nest several years. In the latter category are 256 x 256 HgCdTe SWIR arrays and 256 x 256 InSb arrays, both for operation in the 1-4.8 micron range. In general, is is anticipated that design goal for arrays for ground-based facilities in the 1-30 micron range will possess the largest feasible formats, while longer wavelengths will be addressed by small arrays of individual bolometers or photoconductors.
McLean Ian S.
Wade Richard
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