Fig. 7.
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Examples of synthetic MILES spectra (top panel) for two model galaxies in the CR-IGIMF run of GAEA. The black and gray curves correspond to a high- (M⋆ ∼ 11.3) and low-mass (M⋆ ∼ 9) galaxy, respectively. The bottom panel shows the ratio of each spectrum to that obtained for an MW IMF. Both spectra are at the nominal resolution of MILES (∼2.5 Å FWHM).
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