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A New Deep VLA Radio Survey at 6 cm

Published online by Cambridge University Press:  30 March 2016

K. I. Kellermann ,
E. B. Fomalont ,
D. Weistrop  and
J. Wall
K. I. Kellermann
Affiliation:
National Radio Astronomy Observatory
E. B. Fomalont
Affiliation:
National Radio Astronomy Observatory
D. Weistrop
Affiliation:
Applied Research Corporation
J. Wall
Affiliation:
Greenwich Observatory

Extract

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We have made a new deep 6 cm survey with the VLA in order to extend the radio source count to a lower flux density and to decrease the limits on the small scale fluctuations in the microwave background. The survey region covers ~10-5 ster and is nearly coincident with the survey previously reported by Fomalont et al. 1984a and 1984b. Both the observing time and bandwidth were increased by a factor of two over the previous survey to give a factor of two improvement in sensitivity.

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. 367 - 369
Copyright
Copyright © Reidel 1986

References

Condon, J. J. and Mitchell, K. J. 1984 Astron. J. 89, 610.Google Scholar
Fomalont, E. B., Kellermann, K. I., and Wall, J. V. 1984a Astrophys. J. (Lett.) 277, L23.Google Scholar
Fomalont, E., Kellermann, K. I., Wall, J. V., and Weistrop, D. 1984b Science 225, 23.Google Scholar
Mitchell, K. J. and Condon, J. J. 1985 Astron. J. 90, 1957.Google Scholar
Oort, M.J.A. and Windhorst, R.F A. 1985 Astron. and Astrophys. 145. 405.Google Scholar
Uson, J. M. and Wilkinson, D. T. 1984 Nature 312, 427.Google Scholar