Discussion

does depend on inclination.

• Optical depth effects appears to attenuate FUV more quickly than FIR.

• Bulge-to-Disk may also play a role.

does depend on K-band luminosity.

• Function of stellar populations: Early-type galaxies have a greater percentage of dust heated by optical/NIR photons.

• Early-types have SFR overestimated with FIR, Late-types have SFR underestimated by SFR.