Cambridge Low Frequency Synthesis Telescope
The Cambridge Low-Frequency Synthesis Telescope (CLFST) is an east-west aperture synthesis radio telescope currently operating at 151 MHz. It consists of 60 tracking yagis on a 4.6 km baseline, giving 776 simultaneous baselines. These provide a resolution of 70×70 cosec (declination) arcsec2, with a sensitivity of about 30 to 50 mJy/beam, and a field of view of about 9°×9°. The telescope is situated at the Mullard Radio Astronomy Observatory.
|  Surviving Yagi antennas of the CLFST in June 2014 | |
| Part of | Mullard Radio Astronomy Observatory  | 
|---|---|
| Location(s) | Cambridge, Cambridgeshire, East of England, England | 
| Coordinates | 52°10′13″N 0°02′33″E | 
| Wavelength | 38, 151 MHz (7.89, 1.99 m) | 
| Telescope style | radio telescope  | 
| Website | www | 
|   Location of Cambridge Low Frequency Synthesis Telescope | |
|  Related media on Wikimedia Commons | |

CLFST in May 1999
The CLFST has made three astronomical catalogues of the Northern Hemisphere:
    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.