Fig. 15.
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Relative error on the bulge-to-total ratio in the r band (B/Terr)/(B/T) as a function of B/T for EFIGI galaxies with Incl-Elong ≤ 2, the color of the points indicating the galaxy Hubble type. There is a trend of lower B/T (that correspond to later-type galaxies) showing higher relative errors. All errors are small enough to not alter the results of the present analysis.
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