Identifying AGNs from X-ray Detections: Primary Parameter Calibrations
Introducing novel semi-empirical metallicity calibrations for AGNs that establish intrinsic 2-10 keV X-ray luminosity as the primary input parameter.
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Introducing novel semi-empirical metallicity calibrations for AGNs that establish intrinsic 2-10 keV X-ray luminosity as the primary input parameter.
Investigating the metallicity-luminosity relation in Seyfert galaxies by combining optical emission line datasets with advanced CLOUDY photoionization models.