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Latest revision Your text
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{{Use dmy dates|date=April 2022}}

{{Infobox telescope}}

{{Infobox telescope}}

[[File:Barton_geograph-3763647-by-Ben-Brooksbank.jpg|thumb|left|250px|CLFST in May 1999]]

[[File:Barton_geograph-3763647-by-Ben-Brooksbank.jpg|thumb|left|250px|CLFST in May 1999]]



The '''Cambridge Low-Frequency Synthesis Telescope''' (CLFST) is an east-west [[aperture synthesis]] [[radio telescope]] currently operating at 151 [[Megahertz|MHz]]. It consists of 60 tracking [[yagi antenna|yagis]] on a 4.6&nbsp;km baseline, giving 776 simultaneous baselines. These provide a resolution of 70×70 cosec (declination) arcsec<sup>2</sup>, 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 '''Cambridge Low-Frequency Synthesis Telescope''' (CLFST) is an east-west [[aperture synthesis]] [[radio telescope]] currently operating at 151 [[Megahertz|MHz]]. It consists of 60 tracking [[yagi antenna|yagis]] on a 4.6 km baseline, giving 776 simultaneous baselines. These provide a resolution of 70×70 cosec (declination) arcsec<sup>2</sup>, 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 catalogue]]s of the Northern Hemisphere:

The CLFST has made three [[astronomical catalogue]]s of the Northern Hemisphere:

* [[Sixth Cambridge Survey of radio sources|6C]] survey at 151&nbsp;MHz

* [[Sixth Cambridge Survey of radio sources|6C]] survey at 151 MHz

* [[Seventh Cambridge Survey|7C]] survey at 151&nbsp;MHz

* [[Seventh Cambridge Survey|7C]] survey at 151 MHz

* [[Eighth Cambridge Survey|8C]] survey at 38&nbsp;MHz

* [[Eighth Cambridge Survey|8C]] survey at 38 MHz



[[Category:Radio telescopes]]

[[Category:Radio telescopes]]

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