Fig. 1.
S 24/S 500 vs. S 3.6/S 500, illustrating the diagnostic ratios used by Rowan-Robinson et al. (2014) to select lensed objects, here plotted for the sources in HerMES (Lockman+XMM+ELAIS S1+CDF-S+ELAIS N1) with 0.15 < z < 0.95. Red filled circles: lensed galaxy candidates, large black filled circles: galaxies with standard cirrus components, blue filled circles: galaxies with cool cirrus components, magenta filled circles: galaxies in Lockman with cold cirrus components, small black dots: non-cirrus galaxies.
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