Fig. 7.
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Collage of all LLAMA non-AGN X-shooter spectra with best-fitting stellar population synthesis overplotted. To the right of each spectrum, the summarised stellar population vector shows the best-fitting light-weighted fractions of the young (blue), young-intermediate (green), intermediate-old (yellow), and old (red) populations with boundaries of log (age/years) at 7.5, 8.5, and 9.5.
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