I am studying with Prof. Jeremy Mould, observing active galactic nuclei and their associated super-massive black holes, specifically looking at the dust and gas surrounding and obscuring the central engine.
Using near infrared integral field spectroscopy, the kinematics, distribution and other physical parameters of these features can be determined. We will use large telescopes with infra-red integral field spectroscopy with high spatial resolution, on samples of nearby radio source galaxies.
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