Synopsis of results obtained for the LTG NGC 0776 (D = 65.5 Mpc; log(ℳ_⋆/M_⊙) = 11.1) from spectral modeling of CALIFA IFS data. (a) True-color SDSS image composite of the galaxy. The circle depicts the isophotal diameter of the bulge (153; Breda 2019). (b) EW(Hα) map of the galaxy displayed in the range between 0.5 Å and 57 Å. The vertical bar corresponds to a projected scale of 5 kpc. (c) Radial EW(Hα) profile, with dots showing determinations for single spaxels inside and outside R_B (red and blue, respectively) and squares corresponding to the mean EW(Hα) within irregular isophotal annuli (isan) adapted to the morphology of the emission-line-free stellar continuum (see BP18 for details). Error bars show the standard deviation about the mean of single-spaxel determinations within each isan. The shaded gray horizontal stripe between 0.5 and 2.4 Å marks the range in EW(Hα) that can be accounted for by photoionization by the evolved (> 100 Myr) post-AGB stellar component (e.g., Cid Fernandes et al. 2011; Gomes et al. 2016a). (d) g-band SBPs of the galaxy after the suppression of stellar populations with ages younger than 0.03, 0.1, 0.3, 1, 3, 5, 7, and 9 Gyr (cf. the color-coding at the top right) from CALIFA IFS data. The profile for t_cut = 0 (black) corresponds to the SBP that would be obtained when nebular line emission alone were removed.