Fig. 6.
Star formation rate distribution. The blue and red histograms refer to the unabsorbed and absorbed sources, respectively. The histograms have been normalised to the total number of sources. Left: distributions for the total number of sources. The two populations have similar SFR distributions (p-value = 0.95). Right: distributions for the 1276 AGNs with Herschel photometry available. The X-ray absorbed and unabsorbed AGNs have similar SFR distributions (p-value = 0.86).
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