Difference between revisions of "Dark Energy Camera"

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  |image_text= The 4m Blanco telescope with the DECam (black cylinder) at its prime focus
 
  |image_text= The 4m Blanco telescope with the DECam (black cylinder) at its prime focus
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  |image_text= A sample DECam image of the Small Magellanic Cloud<br>illustrates its tiled CCD array
 
  |image_text= A sample DECam image of the Small Magellanic Cloud<br>illustrates its tiled CCD array
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  |image_by= Dark Energy Survey Collaboration
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Revision as of 04:08, 5 February 2015

The Dark Energy Camera or DECam created at Fermilab became the biggest digital camera in the world[1] when it entered service in 2012[2] at the 4 -meter Blanco telescope of the Cerro Tololo Inter-American Observatory in Chile.

The camera was designed as the research instrument for the Dark Energy Survey, which uses repeated wide-field astronomical observations to shed light on fundamental questions in cosmology.

As this camera was designed for observations of highly-redshifted light, it uses special CCD chips, developed by the Lawrence Berkeley National Laboratory and manufactured by Dalsa. These have a large 15µm-square pixel size, and an extra-deep silicon substrate to maximize photon-capture efficiency at far red wavelengths.

The primary imaging area is a mosaic of 62 CCDs, each of 2048 x 4096 pixels, for 520 megapixels in total. At the edges of the focal plane, twelve additional CCDs of 2048 pixels square are dedicated to focus calibration and guide-star tracking. These extra 50 megapixels are included in the description of the DECam as a "570 megapixel camera" (as typically quoted in publicity materials). The CCD array is cooled to -100°C to reduce thermal noise, held within a vacuum chamber to prevent condensation from forming. Each exposure results in a file size of around a gigabyte, and takes 17 seconds to read out from the sensor[3].

Starlight reflected off the 4-meter-diameter mirror surface passes through corrector optics consisting of five lenses; the largest of these is almost a meter in diameter and weighs 173 kg (380 lbs)[3]. Combined, the whole optical system has an effective focal length of about 11,600 mm and works at f/2.9. With the corrector-optics assembly and filter changer, the camera's complete weight is 4 or 5 tons[4]. The complete camera is somewhat larger than a telephone booth[5].

After checkout and calibration was completed, the Dark Energy Survey observation campaign officially began on August 31, 2013[6]. The full survey project will take five years to complete.

The title of "world's largest digital camera" may eventually pass to the LSST Camera, a somewhat similar design with a planned 3,200 megapixel resolution.


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