Fig. 4.
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Observed near-infrared to millimeter SEDs and best-fit models derived from CIGALE SED fitting analysis of E and W galaxies. Blue line: Best-fit model for the E galaxy. Red line: best-fit model for the W galaxy. Circles: observed fluxes for the E and W galaxies. Triangles: observed upper limits for the E and W galaxies. Observed quantities used in the fit are given in Table 2.
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