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.
| Location(s) | United Kingdom |
|---|---|
| Coordinates | 52°09′58″N 0°02′02″E |
| Telescope style | cosmic microwave background experiment radio telescope |
| | |
Cosmic microwave background radiation (CMB) | |||||||
|---|---|---|---|---|---|---|---|
| |||||||
| Effects |
| 9-year WMAP image (2012) of the CMB. | |||||
| Experiments |
| ||||||
This article about a specific observatory, telescope or astronomical instrument is a stub. You can help Wikipedia by expanding it. |
This physical cosmology-related article is a stub. You can help Wikipedia by expanding it. |