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Email:
F.Shankar@soton.ac.uk

Professor Francesco Shankar 

Francesco Shankar is Professor of Astrophysics and CHEP teaching champion in the School of Physics and Astronomy.

After obtaining his PhD at SISSA and a postdoc at the Ohio State University, he moved to the Max Planck Institute for Astrophysics as an Alexander von Hulmboldt Fellow, and then to the Observatoire de Paris as a Marie Curie Fellow. He then joined the Department of Physics and Astronomy in 2013.

Professor Shankar is PI of a H2020 Marie Skłodowska-Curie Innovative Training Network (https://www.bid4best.org/), fellow of the Alan Turing Institute, fellow of the Higher Education Academy, fellow of the Royal Astronomical Society, and PI of a large-scale project in medical science aimed at optimising blood pressure measurements strategies. Professor Shankar also sits on diverse scientific Advisory Board Panels worldwide and is leading a massive outreach/public engagement project named Astera (Astera - A Cosmological Visualizer (soton.ac.uk)), an interactive, fully immersive 3D realization of the Universe. 

Research

Teaching

Publications

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Research

Research interests

Professor Shankar's research revolves around the theoretical modelling of galaxies, their central supermassive black holes, and their host dark matter haloes. He pioneered in the phenomenological modelling of galaxies and black holes based on a combination of abundance matching and continuity equation techniques. He has now started a group in extra-galactic astronomy aimed at specifically constraining the evolutionary channels of early-type, bulged galaxies and supermassive black holes via advanced semi-empirical models. The latter are characterized by a “bottom-up” approach: The least possible assumptions and associated parameters are initially included in the models which are otherwise informed by a number of independent observations. Additional degrees of complexities can be gradually included wherever needed. Semi-empirical models in this respect are a very powerful complementary tool to cosmological hydrodynamic simulations and semi-analytic models. The team is part of Euclid, Athena, and LSST. The increasing quantity of future data in extra-galactic Astronomy will have to be paralleled by fast modelling. The extreme flexibility and accuracy make semi-empirical models ideal tools to create full test catalogues for fast predictions and comparisons to data. Professor Shankar's research interests also lie in other areas of physics. He acted as guest editor for a review on keV sterile neutrinos and joined as co-I massive grant proposals that focus on the detection of dark matter particles via quantum sensors.

Teaching

Professor Shankar is currently the module leader of Cosmology. In previous years he was teaching Introduction to Astronomy, Galaxies and Photons in Astrophysics.

Publications

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