Fig. 9.
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SFRnorm vs. X-ray luminosity. SFRnorm values are estimated using the expression of Schreiber et al. (2015) to measure the SFRs of star-forming MS galaxies. SFRnorm and LX are the median values of our binned measurements, in bins of LX, with 0.5 dex width. The errors are calculated using bootstrap resampling by performing 100 resamplings with replacement at each bin. The results are colour-coded based on the redshift interval.
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