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Cambridge Low-Frequency Synthesis Telescope : ウィキペディア英語版
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.
The CLFST has made three astronomical catalogues of the Northern Hemisphere:
* 6C survey at 151 MHz
* 7C survey at 151 MHz
* 8C survey at 38 MHz
==External links==

*(Cambridge Low Frequency Synthesis Telescope (CLFST) ) on the internet


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Cambridge Low Frequency Synthesis Telescope」の詳細全文を読む



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