![]() | |
Location(s) | United Kingdom |
---|---|
Coordinates | 52°09′58″N0°02′02″E / 52.166°N 0.034°E |
![]() | |
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. [1] In 1995, it was the first instrument to measure small-scale structure in the cosmic microwave background. [2] [3] When the more sensitive Very Small Array came online in 2000, the CAT was decommissioned and partly dismantled. [4]