CORDIS Project
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This project develops a method to measure black hole masses and accretion rates in distant and obscured active galactic nuclei using infrared spectra from space telescopes. By analyzing gas emission lines, the research aims to establish a connection between black hole properties and stellar kinematics, enhancing our un…
The goal of this proposal is to establish a method for the quantification of fundamental active galactic nucleus (AGN) properties, i.e., black hole (BH) masses and accretion rates, in high-redshift and obscured AGN.
We aim to use infrared spectra from the Spitzer and Herschel space telescopes to study the kinematics and fluxes of gas emission lines originating from the AGN narrow-line region (NLR).
Our first results indicate that the mid-infrared (MIR) NLR line widths follow the relation between…
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