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Fig. 9


Far-infrared radio correlation of our sources, as discussed in Sect. 8. μFIR and μ1.4 correspond to the magnification factors appropriate for the dusty and 1.4 GHz synchrotron emission, respectively. Solid blue and red lines show the relationship for q = 2.4 and 2.0, respectively, while the red dotted line is for q = 2.7. The dot-dashed lines show the ±1σ scatter about q = 2.4 at low redshift from Jarvis et al. (2010).

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