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Fig. 8.

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Surface brightness profiles from elliptical isophotal fits for hosts of radio galaxies 10913 (top panel) and 44 (bottom panel). In both panels, the best-fit Sérsic model, fit to Halo-truncated data within R ∼ 6 kpc (for 10913) and R ∼ 2.8 kpc (for 44) is shown as a solid black line, with best-fit parameters reported in the legend. It closely follows the de Vaucouleurs profile (dashed red line). The Sérsic fit on the full dataset is shown as a solid gray line. The upper x-axis represents the corresponding radius R in pixels, and the y-axis is the ST magnitude per arcsec2.

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