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Fig. 14
Zoom in of a section of the K-band (2.19−2.42 μm) for the comparison of our three models with those of Conroy & van Dokkum (2012, C12) and Maraston et al. (2009, M09), at solar metallicity and 11 Gyr. The spectra are normalised to unity at 1.65 μm and convolved to 20 Å.
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