Fig. D.1.
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Enclosed luminosity (left) and mass (right) profiles constructed from the stellar-light MGE models derived from the HST/WFPC2 F814W image, assuming M/LF814W = 8.4 M⊙/L⊙ (Table 1), and from the HST/NICMOS NIC3 F160W image, assuming M/LF160W = 3.4 M⊙/L⊙ (Table D.1). Profiles are plotted at their widest radial extends, i.e., ≈50″ for the WFPC2 F814W and ≈25″ for the NICMOS F160W images.
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