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Fig. 5.


Fraction of star-forming galaxies identified as LoTSS jellyfish for each cluster. Error bars are 1σ binomial confidence intervals (Cameron 2011). In order to ensure a fair comparison from cluster to cluster, jellyfish fractions in this plot are measured using only galaxies with Mstar > 109.7M and only include jellyfish galaxies identified from the degraded LoTSS imaging.

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