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Westerbork Surveys of Radio Sources at 610 and 1415 MHz

Published online by Cambridge University Press:  14 August 2015

A. G. Willis ,
C. E. Oosterbaan ,
R. S. Le Poole ,
H. R. de Ruiter ,
R. G. Strom ,
E. A. Valentijn ,
Sterrewacht Leiden ,
P. Katgert  and
J. K. Katgert-Merkelijn
A. G. Willis
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
C. E. Oosterbaan
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
R. S. Le Poole
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
H. R. de Ruiter
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
R. G. Strom
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
E. A. Valentijn
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
Sterrewacht Leiden
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
P. Katgert
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna
J. K. Katgert-Merkelijn
Affiliation:
Laboratorio di Radioastronomia CNR, Bologna

Extract

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The Westerbork Synthesis Radio Telescope (WSRT) has now been used to make source surveys at frequencies of 610 and 1415 MHz. This paper summarizes the results concerning source counts and anisotropies in the distribution of sources from those surveys not concerned with clusters of galaxies.

Type
I. Surveys of Radio Sources, Source Counts and Anisotropies
Information
Symposium - International Astronomical Union , Volume 74: Radio Astronomy and Cosmology , 1977 , pp. 39 - 45
Copyright
Copyright © Reidel 1977 

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