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Fig. 13.

image

Top panel: SED for NGC 5257. Bottom panel: SED for NGC 5258. A SED compiled using stellar synthesis model CIGALE (Noll et al. 2009) has been fitted to each SED. Empty blue squares correspond to observed fluxes, red dots indicate model fluxes, and the black solid line corresponds to the model spectrum. Bottom plots: normalized error fit versus wavelength for each galaxy.

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