Fig. B.1
Total infrared (TIR) correlations with Iν(24 μm) for NGC 4567/68, NGC 4501, and NGC 4321. The pixel size is 18″. Residuals of the relations Iν(24 μm) × 3.2 × 10-3/ 8.1 × 10-2 (see Eq. (6)) as a function of TIR1 × 0.46, TIR2 × 0.46, and TIR3 × 0.46 (see Eq. (B.6)). The dashed and dotted lines are at ± 1 × rms in the same color as the corresponding galaxy.
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