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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

Rogier A. Windhorst
Rogier A. Windhorst*
Affiliation:
Mount Wilson and Las Campanas Observatories, The Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101-1292, U.S.A.

Extract

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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.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 355 - 366
Copyright
Copyright © Reidel 1986

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