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Experimental Astronomy

, Volume 3, Issue 1–4, pp 235–238 | Cite as

Infrared astronomy: From one to one million pixels

  • Ian Mclean
Article

Abstract

In less than a decade, infrared “array” detectors have revolutionized infrared astronomy. Most of us remember using single element photometers in the early eighties, yet today, most of us are using 256×256 pixel arrays. At this meeting we have heard of plans to fabricate 1024×1024 arrays in the near infrared. From one to one million pixels in such a short period of time is amazing. The new array technology has also stimulated the development of many varieties of infrared cameras and spectrometers. At the UCLA Infrared Imaging Detector Lab we have commissioned two near infrared imaging systems (KCam and Gemini) based on 256×256 arrays and a spectrometer design study is in progress for 1024×1024 arrays. Performance of these cameras on the telescope will be reported briefly.

Key words

IR arrays infrared instruments 

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References

  1. Casement, S., McLean, I.S. and Fischer, R.E.: 1993, SPIE Proc 1946, in pressGoogle Scholar
  2. McLean, I.S., Becklin, E.E., Brims, G., Canfield, J., Casement, L.S., Figer, D.F., Henriquez, F., Huang, A., Liu, T., Macintosh, B., Teplitz, H.: 1993, SPIE Proc 1946, ir pressGoogle Scholar
  3. PuetterR. and PinaR.: 1993, PASP 105, 630Google Scholar

Copyright information

© Kluwer Academic Publishers 1994

Authors and Affiliations

  • Ian Mclean
    • 1
    • 2
  1. 1.Department of AstronomyUCLALos AngelesUSA
  2. 2.Department of PhysicsUCLALos AngelesUSA

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