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Search for CSS and GPS Candidates from the Peacock and Wall Catalogue

Published online by Cambridge University Press:  05 March 2013

A. Rossetti ,
F. Mantovani ,
C. Fanti  and
R. Fanti
A. Rossetti
Affiliation:
Istituto di Radioastronomia del CNR, via Gobetti 101, I-40129 Bologna, Italy. [email protected]@ira.cnr.it
F. Mantovani
Affiliation:
Istituto di Radioastronomia del CNR, via Gobetti 101, I-40129 Bologna, Italy. [email protected]@ira.cnr.it
C. Fanti
Affiliation:
Istituto di Radioastronomia del CNR, via Gobetti 101, I-40129 Bologna, Italy. [email protected]@ira.cnr.it Dipartimento di Fisica, Università degli Studi, via Irnerio 46, I-40126 Bologna, Italy. [email protected], [email protected]
R. Fanti
Affiliation:
Istituto di Radioastronomia del CNR, via Gobetti 101, I-40129 Bologna, Italy. [email protected]@ira.cnr.it Dipartimento di Fisica, Università degli Studi, via Irnerio 46, I-40126 Bologna, Italy. [email protected], [email protected]
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Abstract

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Samples of CSS/GPS sources suitable for statistical studies have been selected from the 3CR catalogue and from the Peacock & Wall catalogue. The selection criterion used for the Peacock & Wall catalogue CSS/GPS sources selects sources which peak below about 2 GHz and are therefore larger than ˜200 pc. Our main aim is to find among the flat spectrum sources in the Peacock & Wall catalogue smaller size CSS/GPS sources by means of systematic high resolution observations. The discovery of a few more would be important in order to finally have a complete flux limited sample of this class of objects. We discuss the results obtained so far for three of the observed sources.

Keywords

galaxies: activequasars: individual (0153+744, 0133+476, 0202+149)radio continuum: general
Type
GPS/CSS Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 1 , 2003 , pp. 35 - 37
Copyright
Copyright © Astronomical Society of Australia 2003

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