This project will develop model predictions for AGN activity based on a “two-phase” scenario for the growth of supermassive black holes. The model predictions will be tested against available observations, including from the Chandra X-ray Observatory. The funded postdoctoral fellow will be responsible for most of the scientific analysis. The PI will manage the project, and contribute to the analysis and writing up the results
|Effective start/end date
|3/1/22 → 2/29/24
- Smithsonian Astrophysical Observatory (TM2-23005X AMD 1 // NAS8-03060)
- National Aeronautics and Space Administration (TM2-23005X AMD 1 // NAS8-03060)
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