Cambridge Low Frequency Synthesis Telescope
Today, Cambridge Low Frequency Synthesis Telescope is a topic that remains relevant and of interest to a wide audience. Whether due to its impact on society, its historical relevance, or its influence on popular culture, Cambridge Low Frequency Synthesis Telescope continues to be a topic of constant debate and study. From its origins to the present, Cambridge Low Frequency Synthesis Telescope has marked a milestone in different aspects of human life, and its importance remains undeniable. In this article, we will explore the multiple facets of Cambridge Low Frequency Synthesis Telescope and its impact in various areas, with the intention of offering a complete and enriching look at this significant topic.
 Surviving Yagi antennas of the CLFST in June 2014 | |
| Location(s) | Cambridge, Cambridgeshire, East of England, England |
|---|---|
| Coordinates | 52°10′13″N 0°02′33″E / 52.1704°N 0.0426°E |
| Wavelength | 38, 151 MHz (7.89, 1.99 m) |
| Website | www |
  Location of Cambridge Low Frequency Synthesis Telescope | |
 Related media on Commons | |
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.
The CLFST has made three astronomical catalogues of the Northern Hemisphere:
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