Fig. B.1.
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Corner plots obtained from the fitting of a two-dimensional circular model to the SB of the radio halo at 141 MHz (left) and 1.4 GHz (right). The blue lines show the initial estimates for the peak brightness, I0, and the e-folding radius, re, by the pre-MCMC fitting. The x0 and y0 are the best-fit values in R.A. and Dec. of the halo peak.
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