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The Distribution of Faint Radio Sources at 6 cm
Published online by Cambridge University Press: 03 August 2017
Abstract
Deep radio source surveys made with the VLA at 6 cm wavelength show that the radio source count continues to converge down to microjansky flux densities, although there is some evidence of a flattening of the count in the range between 10 and 100 microjansky. The weak sources may be primarily an evolving population of active spiral galaxies.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 379 - 385
- Copyright
- Copyright © Reidel 1988