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Fig. 6


Our data and the 1BB model fit for the epochs 3,5,9, and 10. Overplotted is the AD model, the 1BB model, and the sum of both components. From the data, we observe a clear rise in the blackbody flux, and a clear shift of the blackbody emission peak to shorter wavelengths until epoch 5. This emerging bump is confirmed by the blackbody temperature maximum in epoch 5 of our single-epoch fit (see Fig. 7).

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