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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 17, Iss. 4 — Feb. 15, 1978
  • pp: 574–592

Self-scanned photodiode array: high performance operation in high dispersion astronomical spectrophotometry

Steven S. Vogt, Robert G. Tull, and Phillip Kelton  »View Author Affiliations


Applied Optics, Vol. 17, Issue 4, pp. 574-592 (1978)
http://dx.doi.org/10.1364/AO.17.000574


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Abstract

We have developed a multichannel spectrophotometric detector system using a 1024 element self-scanned silicon photodiode array, which is now in routine operation with the high-dispersion coudé spectrograph of the University of Texas McDonald Observatory 2.7-m telescope. We discuss operational considerations in the use of such arrays for high precision and low light level spectrophotometry. A detailed description of the system is presented. Performance of the detector as measured in the laboratory and on astronomical program objects is described, and it is shown that these arrays are highly effective detectors for high dispersion astronomical spectroscopy.

© 1978 Optical Society of America

History
Original Manuscript: August 6, 1977
Published: February 15, 1978

Citation
Steven S. Vogt, Robert G. Tull, and Phillip Kelton, "Self-scanned photodiode array: high performance operation in high dispersion astronomical spectrophotometry," Appl. Opt. 17, 574-592 (1978)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-17-4-574


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