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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| Format: | Report |
| Language: | unknown |
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arXiv
2003
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| Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0305570 https://arxiv.org/abs/astro-ph/0305570 |