Fig. 14.
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Stacked spectrum of objects selected in lower sequence. Vertical lines show the location of a few usual emission lines (see inside caption). We show the position of the lines, including where the HeI lines would be expected. None of them are detected, confirming these objects do not contain a dominant AGN. This stacked spectrum is similar to that of a young starburst, with a blue UV slope and prominent hydrogen and [OIII) emission lines.
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