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2-Jy Sample of Southern Radio Sources

Published online by Cambridge University Press:  25 May 2016

R. Morganti ,
C.N. Tadhunter ,
R. Dickson ,
M. Shaw ,
T.A. Oosterloo  and
J.E. Reynolds
R. Morganti
Affiliation:
1 Istituto di Radioastronomia, Bologna, Italy
C.N. Tadhunter
Affiliation:
3 Department of Physics, University of Sheffield, UK
R. Dickson
Affiliation:
3 Department of Physics, University of Sheffield, UK
M. Shaw
Affiliation:
3 Department of Physics, University of Sheffield, UK
T.A. Oosterloo
Affiliation:
2 Australia Telescope National Facility, Epping, Australia
J.E. Reynolds
Affiliation:
2 Australia Telescope National Facility, Epping, Australia

Extract

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We have collected multi-waveband (radio, optical and X-ray) data for a complete sample of southern radio sources. The sample includes 88 objects selected from the Wall & Peacock (1985) catalogue that is complete down to S 2.7GHz = 2 Jy, δ < 10° and the z < 0.7. This database (Tadhunter et al. (1993), Morganti et ai. (1993), and Siebert et al. these Proceedings) provides an important tool for investigating the nature of anisotropies and orientation effects in AGN and the physical causes of the correlation between their emission at different frequencies.

Type
Surveys of Radio Sources
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 515 - 516
Copyright
Copyright © Kluwer 1996 

References

Laing, R.A. 1994, in ASP Conf. Ser. 54, p227;Google Scholar
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Tadhunter, C.N., Morganti, R., di Serego Alighieri, S., Fosbury, R.A.E. & Danziger, I.J. 1993, MNRAS , 263, 999;CrossRefGoogle Scholar
Wall, J.V. & Peacock, J.A. 1985, MNRAS , 216, 173.CrossRefGoogle Scholar