Fig. 4.
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Left panel: Fitted spectra of the different components of ORC J0356–4216, including ring 1, ring 2, and the host galaxy. The plotted data correspond to the EMU data and the six sub-bands of the MeerKAT observations. We assumed a 10% integrated flux density uncertainty for the EMU data and 4% for the MeerKAT data. Right panel: MeerKAT 1.28 GHz background map showing the different components of the galaxy.
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