Image Details
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).
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.