Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz
Figure 6
SED for AME-G107.1+5.2 including fluxes at 0.408 and 1.42 GHz from the CGPSE catalogue normalised by the flux loss expected in AMI channel 3 and the flux-loss-corrected AMI fluxes. (a) shows a single free-free component plus spinning dust contribution to the SED; (b) shows a fit to the flux densities using a two-component free-free model plus a spinning dust contribution. Please see the text for details.