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Proceedings Paper

State-Of-The-Art Space Telescope Digicon Performance Data
Author(s): 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
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Paper 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.

Paper Details

Date Published: 7 May 1980
PDF: 14 pages
Proc. SPIE 0217, Advances in Focal Plane Technology, (7 May 1980); doi: 10.1117/12.958477
Show Author Affiliations
R. O. Ginaven, Electronic Vision Co. (United States)
J. P. Choisser, Electronic Vision Co. (United States)
L. Acton, Electronic Vision Co. (United States)
W. Wysoczanski, Electronic Vision Co. (United States)
H. R. Alting-Mees, Electronic Vision Co. (United States)
R. D. Smith II, Electronic Vision Co. (United States)
E. A. Beaver, University of California (United States)
H. J. Eck, Ball Aerospace Systems Division (United States)
A. Delamere, Ball Aerospace Systems Division (United States)
J. L. Shannon, National Aeronautics and Space Administration (United States)

Published in SPIE Proceedings Vol. 0217:
Advances in Focal Plane Technology
William S. Chan, Editor(s)

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