Fig. 7.

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Low frequency radio luminosity versus SFR relation. LOFAR 144 MHz luminosity versus SFR for the Perseus jellyfish galaxies presented in this work (large blue symbols, same marker types as Fig. 1) and the larger low-z LOFAR jellyfish galaxy sample from Roberts et al. (2021a) (gray triangles). We also show the best-fit powerlaw relationships for the jellyfish sample from Roberts et al. (2021a) (solid gray) and the low-z star-forming galaxy sample from Gürkan et al. (2018) (dashed black).
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