Fig. 7.

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Full-resolution (7.6″ × 7.4″) MGCLS Stokes-I intensity image of a multi-host structure in the field of Abell 209. We indicate the two possible intersecting multi-component radio galaxies (giant radio galaxy and a distorted tailed galaxy). The compact radio components circled in green indicate the positions of the likely optical hosts, while the magenta circles indicate other superposed or nearby compact radio emission with optical counterparts. The brightness scale is logarithmic and saturates at 1 mJy beam−1. The synthesised beam is indicated in the lower right corner.
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