Fig. 6.
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Surface brightness, colour and stellar mass density profiles of NGC 1042 using LBT, Dragonfly and SDSS which have different depths. The surface brightness profiles shown here correspond to the observed values while the radial colour and stellar mass density profiles are shown after being corrected by Galactic extinction and the inclination of NGC 1042. In the case of the surface brightness profiles, only values above 3σ the sky noise of the image are shown.
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