Results with the UKIRT infrared camera

Details Results with the UKIRT infrared camera Results with the UKIRT infrared camera

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987spie..782..138m&link_type=abstract

IN: Infrared sensors and sensor fusion; Proceedings of the Meeting, Orlando, FL, May 19-21, 1987 (A88-51054 22-35). Bellingham,

Astronomy and Astrophysics

Astronomy

Cameras, Infrared Astronomy, Semiconductor Devices, Telescopes, Galactic Nuclei, High Resolution, Imaging Techniques, Indium Antimonides, Orion Nebula

Scientific paper

Recent advances in focal plane array technology have made an immense impact on infrared astronomy. Results from the commissioning of the first infrared camera on UKIRT (the world's largest IR telescope) are presented. The camera, called IRCAM 1, employs the 62 x 58 InSb DRO array from SBRC in an otherwise general purpose system which is briefly described. Several imaging modes are possible including staring, chopping and a high-speed snapshot mode. Results to be presented include the first true high resolution images at IR wavelengths of the entire Orion nebula.

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