Fig. 1.
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Best-fit population-orbit superposition model of FCC 177. From top to bottom: maps of the data, model, and residuals (model−data). From left to right: maps of the surface-brightness, SB, mean velocity, V, velocity dispersion, σ, Gauss-Hermite coefficients h3 and h4, light-weighted age and metallicity of the stars. Similar plots for the other sample galaxies are shown in Figs. B.1–B.19.
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