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Deep ATLAS Radio Observations of the Chandra Deep Field–South/Spitzer Wide‐Area Infrared Extragalactic Field

  • Authors: Ray P. Norris, José Afonso, Phil N. Appleton, Brian J. Boyle, Paolo Ciliegi, Scott M. Croom, Minh T. Huynh, Carole A. Jackson, Anton M. Koekemoer, Carol J. Lonsdale, Enno Middelberg, Bahram Mobasher, Seb J. Oliver, Mari Polletta, Brian D. Siana, Ian Smail, and Maxim A. Voronkov

Norris et al. 2006 The Astronomical Journal 132 2409.

  • Provider: AAS Journals

Caption: Fig. 4.

Observed 20 cm integrated flux plotted against SWIRE 24 μm flux for those sources in our sample that were also detected at 24 μm, classified according to the criteria discussed in § 3.4. The diagonal line shows the radio‐FIR correlation ﹩q_{24\,\mu \mathrm{m}\,}=\mathrm{log}\,( S_{24\,\mu \mathrm{m}\,}/ S_{20\,\mathrm{cm}\,}) =0.84﹩ suggested by the Appleton et al. data (2004).

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