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VLA Observations of the Cambridge-Cambridge Rosat Survey

Published online by Cambridge University Press:  25 May 2016

P. Ciliegi ,
M. Elvis ,
B.J. Wilkes ,
B.J. Boyle ,
R.G. Mcmahon  and
T. Maccacaro
P. Ciliegi
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, USA Institute of Astronomy, Cambridge, UK Osservatorio Astronomico di Brera, Milano, Italy
M. Elvis
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, USA Institute of Astronomy, Cambridge, UK Osservatorio Astronomico di Brera, Milano, Italy
B.J. Wilkes
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, USA Institute of Astronomy, Cambridge, UK Osservatorio Astronomico di Brera, Milano, Italy
B.J. Boyle
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, USA Institute of Astronomy, Cambridge, UK Osservatorio Astronomico di Brera, Milano, Italy
R.G. Mcmahon
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, USA Institute of Astronomy, Cambridge, UK Osservatorio Astronomico di Brera, Milano, Italy
T. Maccacaro
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, USA Institute of Astronomy, Cambridge, UK Osservatorio Astronomico di Brera, Milano, Italy

Extract

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We report the result of the VLA observations of all the 80 AGN in the Cambridge-Cambridge ROSAT Serendipity Survey (CRSS, Boyle et al. 1995), a new well defined sample of 80 X-ray selected AGN with fx (0.5-2.0keV)≥ 2 × 10–14 erg s–1 cm–2. Our aim was to obtain a complete classification of the sample members as Radio-loud (RL) or Radio-quiet (RQ) in order to determine well-constrained X-ray luminosity function (XLF) for X-ray selected RQ and RL AGN separately.

Type
Cosmological Implications
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 543 - 544
Copyright
Copyright © Kluwer 1996 

References

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