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Is the Upturn in the Source Counts Caused by Primeval Radio Galaxies?
Published online by Cambridge University Press: 30 March 2016
Extract
During the last decade several deep surveys have been made with various aperture synthesis radio telescopes. At milliJansky levels important contributions were made with the WSRT 3 km array and the Cambridge One Mile Telescope. At sub-milliJansky levels surveys have been done with the VLA and the WSRT down to rms noise values of ~10 μJy.
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- Copyright © Reidel 1986
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