Zoom-in on Mg I] λ4571 in model 13E at 200 days (left) and 300 days (right). The total flux and the contribution by Mg I are plotted. At 200 days there is significant line blocking of the red side of the Mg I emission (as well as a blend with some iron-group line emission). At 300 days both the line blocking and blending have abated.
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