Francesco Shankar

most citedAn Eddington ratio-driven origin for the

L_{X} - M_{*}

relation in quiescent and star forming active galaxies

8 citations · 8 across the 1 of their papers we have counts for

collaborators

2 papers

astro-ph.GA2022★ 8 cited

An Eddington ratio-driven origin for the $L_{X} - M_{*}$ 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 $⟨ L_{X} ⟩$ , and the host galaxy stell…

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…

An Eddington ratio-driven origin for the LX​−M∗​ relation in quiescent and star forming active galaxies

Using Unreal Engine to Visualize a Cosmological Volume

An Eddington ratio-driven origin for the $L_{X} - M_{*}$ relation in quiescent and star forming active galaxies