activity
20172023
most citedThe Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies

79 citations · 463 across the 15 of their papers we have counts for

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13 papers · 1 filter

astro-ph.GA2023★ 9 cited

Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations

N. Menci, F. Fiore, F. Shankar +2

To tackle the still unsolved and fundamental problem of the role of Active Galactic Nuclei (AGN) feedback in shaping galaxies, in this work we implement a new physical treatment of…

astro-ph.GA2021★ 5 cited

The size function of massive satellites from the and relations: constraining the role of environment

Lorenzo Zanisi, Francesco Shankar, Mariangela Bernardi +2

In previous work we showed that a semi-empirical model in which galaxies in host dark matter haloes are assigned stellar masses via a stellar mass-halo mass (SMHM) relation and siz…

astro-ph.GA2021★ 17 cited

The evolution of compact massive quiescent and starforming galaxies derived from the and relations

L. Zanisi, F. Shankar, H. Fu +12

The mean size ( effective radius ) of Massive Galaxies (MGs, ) is observed to increase steadily with cosmic time. It is still unclear whether th…

astro-ph.GA2020★ 48 cited

The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework

C. Foster, J. T. Mendel, C. D. P. Lagos +40

We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical dri…

astro-ph.GA2020★ 67 cited

The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view

Lorenzo Zanisi, Marc Huertas-Company, Francois Lanusse +10

Hydrodynamical simulations of galaxy formation and evolution attempt to fully model the physics that shapes galaxies. The agreement between the morphology of simulated and real gal…

astro-ph.GA2019★ 46 cited

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.GA2019★ 37 cited

Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions

Lorenzo Zanisi, Francesco Shankar, Andrea Lapi +6

The mass and structural assembly of galaxies is a matter of intense debate. Current theoretical models predict the existence of a linear relationship between galaxy size () an…

astro-ph.GA2019★ 3 cited

Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency

Francesco Shankar, Viola Allevato, Mariangela Bernardi +11

A supermassive black hole has been found at the centre of nearly every galaxy observed with sufficient sensitivity. The masses of these black holes are observed to increase with ei…

astro-ph.GA2019★ 17 cited

Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL

Philip J. Grylls, F. Shankar, J. Leja +4

Observational systematics complicate comparisons with theoretical models limiting understanding of galaxy evolution. In particular, different empirical determinations of the stella…

astro-ph.GA2019★ 70 cited

The Main Sequence at contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts?

A. Puglisi, E. Daddi, D. Liu +20

ALMA measurements for 93 -selected galaxies at in COSMOS reveal a sizable (\%) population with compact star formation (SF) sizes, lyi…

astro-ph.GA2018★ 37 cited

A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters

P. J. Grylls, F. Shankar, L. Zanisi +1

We present STEEL a STatistical sEmi-Empirical modeL designed to probe the distribution of satellite galaxies in groups and clusters. Our fast statistical methodology relies on trac…

astro-ph.GA2018★ 79 cited

The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies

A. Lapi, L. Pantoni, L. Zanisi +6

[ABRIDGED] We aim to provide a holistic view on the typical size and kinematic evolution of massive early-type galaxies (ETGs), that encompasses their high- star-forming progeni…

astro-ph.GA2017★ 17 cited

Revisiting the bulge-halo conspiracy II: Towards explaining its puzzling dependence on redshift

Francesco Shankar, Alessandro Sonnenfeld, Philip Grylls +8

We carry out a systematic investigation of the total mass density profile of massive (Mstar~3e11 Msun) early-type galaxies and its dependence on redshift, specifically in the range…