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Fig. 11.
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SFRnorm vs. specific black hole accretion rate (λs, BHAR) for sources in COSMOS and in the Boötes field. Median values are presented and the errors are calculated using bootstrap resampling. In both cases, we observe an increase in SFRnorm with λs, BHAR. This is more evident in the case of the Boötes dataset.
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