Fig. 21
Observed zJ and HK spectra at days 198 and 206 (black) compared to NIR spectra for the preferred model (12F, red) and model 12E (blue), which differs only in that τdust = 0. The observed spectra were flux calibrated with the interpolated observed J, H, and K magnitudes at day 200 and we also show the dust emission component for the preferred model (green).
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