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Fig. 13


Hermes spectral shapes (dotted lines, colors denote the observation epoch) compared to spectral shapes from different atmosphere models convolved to the same resolution. The full black line is the model shown in Fig. 11. The dashed lines have the same parameters, except for the reddening, which is E(B − V) = 0.12 and 0.02 for the lower and upper line, respectively.

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