Relation between AGN type and host galaxy properties

We use 3,213 Active Galactic Nuclei (AGNs) from the $\it{XMM}$-XXL northern field to investigate relation of AGN type with host galaxy properties. Applying a Bayesian method, we derive hardness ratios (HRs) and through these hydrogen column density ($\rm N_H$) for each source. consider as absorbed sources (type-2) those $\rm N_H > 10^{21.5}\, \rm{cm^{-2}}$. examine star formation rate (SFR) well stellar mass (M$_*$) distributions both unabsorbed sources. Our work indicates that there is no significant link between Next, whether power, represented by its X-ray luminosity, L_X$, correlates any deviation galaxy's place so-called Main Sequence galaxies, this separately obscured unobscured populations. To take into account effect M$_*$ redshift on SFR, normalised SFR (SFR$_{norm}$). find correlation L_X$ SFR$_{norm}$, follows approximately same trend sources, result favours standard unification models. Finally, explore connection obscuration, N_H$, SFR. these, suggesting obscuration not related large scale in galaxy.