Fig. 28.
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Log ratio of radio-to-FIR flux densities for 49 star-forming cluster galaxies in Abell 209 as a function of projected radius from the cluster centre in units of R200. Black circles indicate the star-forming galaxies in the Abell 209 cluster that have MGCLS radio and Herschel FIR flux densities. All error bars are 1σ uncertainties. The red line is the weighted least-squares fit given in Eq. (7), with the grey region showing the 1σ uncertainty of the fit.
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