Fig. C.1.
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NGC 5128 surface brightness profiles from van den Bergh (1976, magenta line and dots, converted into μB) and Dufour et al. (1979, solid black line) extended outward using the fits to the star counts from Paper I. The red line is from the power-law fit to the star counts, while the blue line is from a de Vaucouleurs r1/4 law fit to the starcounts.
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