Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-27T21:11:00.518Z Has data issue: false hasContentIssue false

Near-IR properties of Spitzer sources

Published online by Cambridge University Press:  01 August 2006

Eduardo A. Gonzalez-Solares
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK email: [email protected], [email protected]
Nicholas A. Walton
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK email: [email protected], [email protected]
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: [email protected]
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Dye, S., Warren, S. J., Hambly, N. C., et al. 2006, MNRAS, 372, 1227CrossRefGoogle Scholar
Lonsdale, C. J., Smith, H. E., Rowan-Robinson, M., et al. 2003, PASP, 115, 897CrossRefGoogle Scholar
Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., et al. 2006, ApJS, 162, 38CrossRefGoogle Scholar