papers

Publications (11)

astro-ph.GA2022

An Eddington ratio-driven origin for the relation in quiescent and star forming active galaxies

Rosamaria Carraro, Francesco Shankar, Viola Allevato +5

A mild correlation exists in active galaxies between the mean black hole accretion, as traced by the mean X-ray luminosity , and the host galaxy stell…

astro-ph.GA2019

Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nuclei

Francesco Shankar, David H. Weinberg, Christopher Marsden +25

The masses of supermassive black holes at the centres of local galaxies appear to be tightly correlated with the mass and velocity dispersions of their galactic hosts. However, the…

astro-ph.GA2021

The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution

Christopher Marsden, Francesco Shankar, Mariangela Bernardi +3

Velocity dispersion () is a key driver for galaxy structure and evolution. We here present a comprehensive semi-empirical approach to compute via detailed Jeans modelling…

astro-ph.CO2021

Building robust AGN mock catalogs to unveil black hole evolution and for survey planning

Viola Allevato, Francesco Shankar, Christopher Marsden +5

The statistical distributions of active galactic nuclei (AGN), i.e. accreting supermassive black holes (BHs), in mass, space and time, are controlled by a series of key properties,…

astro-ph.GA2020

Using Unreal Engine to Visualize a Cosmological Volume

Christopher Marsden, Francesco Shankar

In this work we present `Astera', a cosmological visualization tool that renders a mock universe in real time using Unreal Engine 4. The large scale structure of the cosmic web is…

astro-ph.CO2022

Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl

Hao Fu, Francesco Shankar, Mohammadreza Ayromlou +19

The relative roles of mergers and star formation in regulating galaxy growth are still a matter of intense debate. We here present our DECODE, a new Discrete statistical sEmi-empir…