Cosmic Anisotropy Telescope
From Wikipedia, the free encyclopedia
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.
[edit] 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
 |
This article about a specific observatory, telescope or astronomical instrument is a stub. You can help Wikipedia by expanding it. |
|
|||||||||||||
