COSMOSFieldX-Ray&FIRDetectedAGNMultiwavelengthPropertiesCatalog

The authors find that the AGN 2-10 keV luminosity (L_X) and the host galaxy 8-1000 um star formation luminosity (L^SF_IR) are significantly correlated. However, the average host L^SF_IR has a flat distribution in bins of AGN L_X, while the average AGN L_X increases in bins of host L^SF_IR, with a logarithmic slope of ~ 0.7, in the redshifts range 0.4 < z < 1.2.

In the reference paper, the authors also discuss the comparison between the distribution of these two quantities and the predictions from hydrodynamical simulations. Finally, they find that the average column density (N_H) shows a positive correlation with the host M_*, at all redshifts, but not with the SFR (or L^SF_IR). This translates into a negative correlation with specific SFR.

These results are in agreement with the idea that BH accretion and SFRs are correlated, but occur with different variability time scales. The presence of a positive correlation between N_H and host M_* suggests that the X-ray N_H is not entirely due to the circumnuclear obscuring torus, but may also include a contribution from the host galaxy. This table summarizes the multiwavelength properties of the 692 AGN-host systems detected in the COSMOS field both in the X-ray and in the FIR (the X-FIR sample).

This table was created by the HEASARC in July 2017, based on <a href="cdsarc.cds.unistra.fr/ftp/cats/J/A+A/602/A123">CDS Catalog J/A+A/602/A123</a> file table1.dat, which contains the multiwavelength properties of the 692 sources in the X-FIR sample. This is a service provided by NASA HEASARC .