Distribution of the angle between the direction of the tail and the direction towards the cluster centre. The tail angle distribution of all jellyfish candidates is given in blue. The distribution of candidates with a spectroscopic redshift matching with the associated cluster membership is shown in orange. The combined distribution of galaxies with no spectroscopic redshift and confirmed cluster membership are shown in red. We note that there are two peaks in distribution at 70° and 160° when we include all the candidates and also for galaxies with no redshift information.