Fig. 11
Accounting for stellar mass effects in SFR-L150 MHz. Left: SFR-L150 MHz relationship with the mass dependence taken out using Eq. (2) and the best-fit parameters. Stellar mass is indicated by the colour bar to the right. Right: same as the left, but with the relationship between the stellar mass and radio luminosity normalised by the SFR using Eq. (2).
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