Research Article

Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz

Figure 5

SED for AME-G107.1+5.2. The fluxes at 0.408 and 1.42 GHz are from the CGPSE catalogue normalised by the flux loss expected in AMI channel 3; the higher frequency fluxes are the flux-loss-corrected AMI fluxes. Two free-free SED components are shown using a source size for the low-frequency component fixed to that measured from the AMI SA maps.
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