Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz
Figure 4
SED for AME-G107.1+5.2. (a) shows the 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. The markers and spectral index fits shown are in Figure 2. (b) shows a fit to the flux densities using a two-component model consisting of a classical and a hypercompact HII region.
