Fig. 3
Estimated bivariate PDF shown on logarithmic scale for the K band with the 250 μm-band, for only late-type galaxies. Crosses correspond to the detected fluxes, while downward-pointing triangles to upper limits. Contour lines correspond to the levels 0.00001, 0.0001, 0.001, 0.01, 0.05, 0.1, 0.3, 0.5, 0.7, 0.9. These values correspond to the fraction of the peak value of the BLF that is set to one. The figure clearly shows the correlation among the data.
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