Morphology and surface photometry of a sample of isolated early-type galaxies from deep imaging

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Fig. 6.

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Comparison between our integrated magnitudes in g and r bands with the SDSS DR16 values reported in Table 2. The solid lines show our errors. KIG 637 is not plotted because the magnitudes are strongly influenced by the nearby bright star HD238370 (see Sect. 4.2).

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