activity
20172022
most citedBlack hole scaling relations of active and quiescent galaxies: Addressing selection effects and constraining virial factors

93 citations · 263 across the 9 of their papers we have counts for

collaborators

16 papers

astro-ph.GA202249 cited

Coincidence between morphology and star-formation activity through cosmic time: the impact of the bulge growth

Paola Dimauro, Emanuele Daddi, Francesco Shankar +10

The origin of the quenching in galaxies is still highly debated. Different scenarios and processes are proposed. We use multi-band (400-1600 nm) bulge-disc decompositions of massiv…

astro-ph.GA20215 cited

The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass

Akke Viitanen, Viola Allevato, Alexis Finoguenov +2

The co-evolution between central supermassive black holes (BH), their host galaxies, and dark matter halos is still a matter of intense debate. Present theoretical models suffer fr…

astro-ph.GA20215 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.GA202117 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

The case for the fundamental - relation

Christopher Marsden, Francesco Shankar, Michele Ginolfi +1

Strong scaling relations between host galaxy properties (such as stellar mass, bulge mass, luminosity, effective radius etc) and their nuclear supermassive black hole's mass point…

astro-ph.GA2020

The significant effects of stellar mass estimation on galaxy pair fractions

Philip J. Grylls, F. Shankar, C. Conselice

There exist discrepancies in measurements of the number and evolution of galaxy pairs. The pair fraction appears to be sensitive to both the criteria used to select pair fraction a…