Meeting the Optical Requirements of Large Focal-Plane Arrays
Technological advances will allow the placement of many Terahertz detectors at the focal plane of a single telescope. For a telescope of a given diameter and wavelength of operation, there is a limit to the number of usable detectors imposed by diffraction and optical aberrations. These effects can...
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Language: | English |
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2003
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Online Access: | http://cds.cern.ch/record/618721 |