Fig. 3.

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Radial profiles for five studied objects (in the cases of elliptical annuli, we consider the major axis for the radial distance). The radio emission with the best-fit model found from Halo-FDCA and errors (shaded) is shown in red; the X-ray emission extracted in the same regions is shown in blue. The red dotted line is the 1σ threshold of the radio images. For PSZ2G066.41+27, we report the 1D profile and the residual image after the subtraction of the elliptical exponential model, with the masked regions in red.
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