Far-IR luminosity vs. dust-absorbed luminosity as estimated from the E(B−V) values derived from SED model A. Our three far-IR detections are marked with magenta stars. Blue triangles show estimates at our approximate detection threshold in the far-IR of L_IR ~ 10^11.8L_⊙. Black triangles show upper limits to the dust absorbed luminosities, and have been shifted by –0.02 dex along the y-axis for clarity. The dotted black line shows the 1:1 relation.