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Fig. 20

image

Observed (black circles) and J14 model pseudo-BCs between days 100 and 500 for the I, z, K, S1, and S2 bands. The model families differing in molecular cooling (complete, red; none, blue) and the optical depth of the dust (0, long-dashed; 0.25, short-dashed; 0.44, solid) are shown. 17 M and medium mixing models are not shown. The error bars arising from the extinction are marked in the upper left or right corner.

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