Fig. 9.

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Bayesian model overview, showing how Alcyoneus’s lobe volumes can be estimated by comparing an observed radio image to modelled radio images. Top: LoTSS DR2 compact-source-subtracted 90″ image of Alcyoneus. Middle: highest-likelihood model image. Bottom: same model image convolved to 90″ resolution, with 2σ and 3σ contours of the observed image overlaid.
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