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Ultradeep Optical Identifications and Spectroscopy of Faint Radio Sources
Published online by Cambridge University Press: 19 July 2016
Extract
During the last two years we have completed an extensive project of direct CCD imaging with the Palomar 200 inch Four-shooter on several milliJansky and microJansky radio samples, now totaling 200 sources. The purpose is to study the nature and redshift distribution of the radio galaxies that cause the upturn in the milliJansky source counts (WMOKK) and to search for candidates of primeval radio galaxies.
- Type
- Chapter IX: The Distribution of Radio Sources
- Information
- Symposium - International Astronomical Union , Volume 124: Observational Cosmology , 1987 , pp. 573 - 576
- Copyright
- Copyright © Reidel 1987
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