(a) NGC 2865 and (b) NGC 4697 SED fits using all continuum detections reported in NED (including, whenever reported, data from Infrared Space Observatory: 60, 90, 170, and 200 μm, IRAS: 60 and 100 μm, MIPS: 70 and 160 μm, SPIRE: 250 and 500 μm, VLA: 1.4 GHz and 8.5 GHz), as well as integrated Band 3 and Bands 3+6 continuum measurements that may not be purely thermal in nature.