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Fig. 1.

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SDSS true-colour images and respective SBPs for three exemplary LTGs, demonstrating the morphological differences of the three ⟨δμ9G⟩ intervals tentatively defined in BP18. The synthetic SBPs were computed by convolving the observed IFS data with the SDSS r-band filter transmission curve after removal with ℛ𝒴 of stellar populations younger than 0.03, 0.1, 0.3, 1, 3, 5, 7, and 9 Gyr, being colour coded according to the age they represent. Shown in grey is the r-band SBP extracted from the SDSS photometric data. The vertical dashed line illustrates the estimated isophotal bulge radius ℛB, depicted in the true colour image by a while circle.

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