Infrared astronomy: From one to one million pixels

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Arrays, Cameras, Infrared Astronomy, Infrared Detectors, Infrared Spectrometers, Infrared Telescopes, Near Infrared Radiation, Astronomical Photography, Astronomical Spectroscopy, Infrared Photography, Infrared Spectroscopy, Mercury Cadmium Tellurides

Scientific paper

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 x 256 pixel arrays. At this meeting we have heard of plans to fabricate 1024 x 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 spectrometes. At the UCLA Infrared Imaging Dectector Lab we have commissioned two near infrared imaging systems (KCam and Gemini) based on 256 x 256 arrays and a spectrometer design study is in progress for 1024 x 1024 arrays. Performance of these cameras on the telescope will be reported briefly.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Infrared astronomy: From one to one million pixels does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Infrared astronomy: From one to one million pixels, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared astronomy: From one to one million pixels will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1871359

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.