Fig. 3.

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SFRnorm vs. X-ray luminosity. SFRnorm and LX are the median values of our binned measurements, in bins of LX, with 0.25 dex width. Errors are calculated using bootstrap resampling by performing 1000 resamplings with replacement at each bin. The dashed horizontal line indicates the SFRnorm value (=1) for which the SFR of AGN is equal to the SFR of star-forming galaxies. SFRnorm values are similar in overlapping LX regardless of redshift. AGN host-galaxies have SFR that is below or similar to the SFR of MS galaxies at LX, 2−10 keV < 1044 erg s−1. At higher X-ray luminosities, SFRnorm increases at both redshift intervals.
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