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.
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Location(s) | United Kingdom ![]() |
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Coordinates | 52°09′58″N 0°02′02″E ![]() |
Telescope style | cosmic microwave background experiment radio telescope ![]() |
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Cosmic microwave background radiation (CMB) | |||||||
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Effects |
| ![]() 9-year WMAP image (2012) of the CMB. | |||||
Experiments |
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