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Fig. 12.

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Results on the two-component modeling via the theoretical formalism for both the elliptical (columns one and three) and spherically symmetric implementations (columns two and four). Here, the shape parameters of the gNFW are frozen to the A10-UPP values. The first two columns are modeled to ALMA+ACA+ACT observations and the last two only to ALMA+ACA. In red, we show the unsmoothed model reconstruction. The color map and black contours are the same reconstruction but smoothed with 5″ Gaussian taper to match the observations. The contours are drawn at the same levels in Figure 11. In purple, we show the contours of Figure 11. This figure indicates that the two-elliptical SZ components better resembles the surface brightness distribution of XLSSC 122 than the spherical one.

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