Cosmic Anisotropy Telescope
![Cosmic Anisotropy Telescope is located in the United Kingdom](http://upload.wikimedia.org/wikipedia/commons/thumb/d/d7/United_Kingdom_relief_location_map.jpg/240px-United_Kingdom_relief_location_map.jpg)
![Cosmic Anisotropy Telescope](http://upload.wikimedia.org/wikipedia/commons/thumb/0/0c/Red_pog.svg/8px-Red_pog.svg.png)
Location of Cosmic Anisotropy Telescope
![](http://upload.wikimedia.org/wikipedia/en/thumb/4/4a/Commons-logo.svg/12px-Commons-logo.svg.png)
[edit on Wikidata]
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
- v
- t
- e
- Cosmic variance
- Diffusion damping
- Recombination
- Sachs–Wolfe effect
- Sunyaev–Zeldovich effect
- Thomson scattering
4-year Planck image (2018) of the CMB.
Space | |
---|---|
Balloon | |
Ground |
|
![]() | This article about a specific observatory, telescope or astronomical instrument is a stub. You can help Wikipedia by expanding it. |
- v
- t
- e
![]() | This physical cosmology-related article is a stub. You can help Wikipedia by expanding it. |
- v
- t
- e