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Cosmic Anisotropy Telescope : ウィキペディア英語版 | Cosmic Anisotropy Telescope
The Cosmic Anisotropy Telescope (CAT) was a three-element interferometer for cosmic microwave background radiation (CMB/R) observations at 13 to 17 GHz, based at the Mullard Radio Astronomy Observatory. In 1995, it was the first instrument to measure small-scale structure in the cosmic microwave background. When the more sensitive Very Small Array came online, the CAT telescope was decommissioned in a ceremonial bonfire. == External links ==
* (Cosmic Anisotropy Telescope (CAT) online ) * (The first detection of small-scale structure ) in the cosmic microwave background * (Press release from 1995 describing first measurements of small-scale structure in the cosmic microwave background ) * (The CAT enclosure ) on Google Maps
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