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Fig. 2

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Comparison between the integrated SCO flux determined by Kuno et al. (2007) and those determined by Helfer et al. (2003; red filled dots), Chung et al. (2009a; blue filled triangles), corrected as described in the text, and the extrapolated fluxes of the FCRAO survey (Young et al. 1995; cyan empty circles), for all HRS galaxies in common, on logarithmic (upper panel) and on linear scales (lower panel). The short dashed black line shows the 1:1 relationships.

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