Paper
20 October 1993 58 x 62 Si:As IBC detector arrays on PMOS multiplexers for astronomy
Mark E. McKelvey, Robert E. McMurray Jr., Craig R. McCreight, Thomas L. Roellig, Robert Cooper, Lunming Yuen, Lynne K. Deutsch
Author Affiliations +
Abstract
Four 58 X 62-element Si:As impurity-band-conduction (IBC) detector arrays produced by the Hughes Technology Center were tested to evaluate their usefulness for space- and ground- based astronomical observations. PMOS circuitry was used in the multiplexers to improve low-temperature noise performance. Laboratory tests at background levels simulating those expected on space-based observing platforms were combined with ground-based telescope IR observations. The devices have shown read noise levels below 120 rms e-, dark currents below 10 e-/s, and detective quantum efficiencies of 20%.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark E. McKelvey, Robert E. McMurray Jr., Craig R. McCreight, Thomas L. Roellig, Robert Cooper, Lunming Yuen, and Lynne K. Deutsch "58 x 62 Si:As IBC detector arrays on PMOS multiplexers for astronomy", Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); https://doi.org/10.1117/12.158663
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Cited by 3 scholarly publications.
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KEYWORDS
Signal to noise ratio

Astronomy

Capacitance

Multiplexers

Telescopes

Cameras

Infrared detectors

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