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Near-IR properties of Spitzer sources

Published online by Cambridge University Press:  01 August 2006

Eduardo A. Gonzalez-Solares ,
Nicholas A. Walton ,
Anita M. S. Richards  and
Jonathan A. Tedds
Eduardo A. Gonzalez-Solares
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK email: eglez@ast.cam.ac.uk, naw@ast.cam.ac.uk
Nicholas A. Walton
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK email: eglez@ast.cam.ac.uk, naw@ast.cam.ac.uk
Anita M. S. Richards
Affiliation:
Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9Dl, UK
Jonathan A. Tedds
Affiliation:
Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK email: jat@star.le.ac.uk
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We present an analysis of the near-IR properties of galaxies and quasars detected in the mid-IR by the Spitzer Space Telescope. Using optical photometry from the Wide Field Survey and near-IR fluxes from the First Data Release of the UKIDSS (Dye et al. 2006) survey we carry out a preliminary characterization of the surface density of different samples of galaxies and their clustering properties.

References

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