activity
20162026
most citedNo significant evolution of relations between Black hole mass and Galaxy total stellar mass up to z~2.5

129 citations · 475 across the 29 of their papers we have counts for

collaborators
Showing 2021Show all

5 papers · 1 filter

astro-ph.GA2021★ 11 cited

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 as…

astro-ph.GA2021★ 24 cited

The Black Hole Mass Function Across Cosmic Times I. Stellar Black Holes and Light Seed Distribution

Alex Sicilia, Andrea Lapi, Lumen Boco +7

This is the first paper in a series aimed at modeling the black hole (BH) mass function, from the stellar to the intermediate to the (super)massive regime. In the present work we f…

astro-ph.GA2021★ 20 cited

Rejuvenation triggers nuclear activity in nearby galaxies

Ignacio Martin-Navarro, Francesco Shankar, Mar Mezcua

Feedback, in particular from active galactic nuclei (AGN), is believed to play a crucial role in the evolution of galaxies. In the local Universe, many galaxies with an AGN are ind…

gr-qc2021

Probing modified gravity with magnetically levitated resonators

Chris Timberlake, Andrea Vinante, Francesco Shankar +2

We present an experimental procedure, based on Meissner effect levitation of neodymium ferromagnets, as a method of measuring the gravitational interactions between mg masses. The…

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,…