Left: SFR_norm − L_X correlation in L_X bins, for absorbed and unabsorbed sources. Based on our measurements the AGN enhances the SFR of the host galaxy at all X-ray luminosities spanned by our sample, regardless of whether the source is X-ray absorbed or not. Right: SFR_norm − L_X correlation in SFR_norm bins, for absorbed and unabsorbed sources (Masoura et al. 2018). Absorbed and unabsorbed sources approximately follow the same trend. In both plots red and blue triangles refer to the absorbed and unabsorbed sources, respectively. The dashed line corresponds to the star-forming main sequence. Median SFR and L_X values are presented in both panels. The error bars represent the 1σ dispersion of each bin. Based on our measurements, the SFR_norm − L_X correlation is similar for different AGN types.