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High-z radio starbursts host X-ray AGN

Published online by Cambridge University Press:  01 August 2006

Anita M. S. Richards
Affiliation:
Jodrell Bank Observatory, University of Manchester, SK11 9DL, UK. amsr@jb.man.ac.uk
R. Beswick
Affiliation:
Jodrell Bank Observatory, University of Manchester, SK11 9DL, UK. amsr@jb.man.ac.uk
S. T. Garrington
Affiliation:
Jodrell Bank Observatory, University of Manchester, SK11 9DL, UK. amsr@jb.man.ac.uk
T. W. B. Muxlow
Affiliation:
Jodrell Bank Observatory, University of Manchester, SK11 9DL, UK. amsr@jb.man.ac.uk
H. Thrall
Affiliation:
Jodrell Bank Observatory, University of Manchester, SK11 9DL, UK. amsr@jb.man.ac.uk
M. A. Garrett
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, The Netherlands
M. Kettenis
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, The Netherlands
H. J. van Langevelde
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, The Netherlands
E. Gonzalez-Solarez
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK.
N. A. Walton
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK.
M. G. Allen
Affiliation:
CDS (UMR 7550), 11 rue de l'Université, 67000 Strasbourg, France.
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Abstract

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We use Virtual Observatory methods to investigate the association between radio and X-ray emission at high redshifts. Fifty-five of the 92 HDF(N) sources resolved by combining MERLIN+VLA data were detected by Chandra, of which 18 are hard enough and bright enough to be obscured AGN. The high-z population of μJy radio sources is dominated by starbursts an order of magnitude more active and more extended than any found at z < 1 and at least a quarter of these simultaneously host highly X-ray-luminous obscured AGN.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

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