Paper
7 May 1980 State-Of-The-Art Space Telescope Digicon Performance Data
R. O. Ginaven, J. P. Choisser, L. Acton, W. Wysoczanski, H. R. Alting-Mees, R. D. Smith II, E. A. Beaver, H. J. Eck, A. Delamere, J. L. Shannon
Author Affiliations +
Proceedings Volume 0217, Advances in Focal Plane Technology; (1980) https://doi.org/10.1117/12.958477
Event: 1980 Los Angeles Technical Symposium, 1980, Los Angeles, United States
Abstract
The Digicon has been chosen by NASA as the detector for two of the focal plane instruments on the Space Telescope. Both detectors are 512 channel, parallel output devices and feature photon-counting capability. Recently, tubes for this application have been fabri-cated and tested at Electronic Vision Company. Using a unique computer-assisted test facility, these tubes have been characterized with respect to diode array performance, photocathode response (1100-9000 Å), and imaging capability. In this paper, data are pre-sented on diode dark current and capacitance distributions, pulse height resolution, photocathode quantum efficiency, uniformity and blemishes, dark count rate, distortion, resolution, and crosstalk. Results indicate that the Space Telescope Digicon is capable of extremely low-noise performance in the pulse counting mode.
© (1980) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. O. Ginaven, J. P. Choisser, L. Acton, W. Wysoczanski, H. R. Alting-Mees, R. D. Smith II, E. A. Beaver, H. J. Eck, A. Delamere, and J. L. Shannon "State-Of-The-Art Space Telescope Digicon Performance Data", Proc. SPIE 0217, Advances in Focal Plane Technology, (7 May 1980); https://doi.org/10.1117/12.958477
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Cited by 2 scholarly publications.
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KEYWORDS
Diodes

Distortion

Sensors

Space telescopes

Quantum efficiency

Ultraviolet radiation

Aerospace engineering

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