activity
20192022
most citedThe Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties

16 citations · 30 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20229 cited

Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations

Iván Muñoz Rodríguez, Antonis Georgakakis, Francesco Shankar +5

This paper explores the role of small-scale environment ( Mpc) in modulating accretion events onto supermassive black holes by studying the incidence of Active Galactic Nuclei…

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.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.GA201916 cited

The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties

V. Allevato, A. Viitanen, A. Finoguenov +10

Aims. We perform clustering measurements of 800 X-ray selected Chandra COSMOS Legacy (CCL) Type 2 AGN with known spectroscopic redshift to probe the halo mass dependence on AGN hos…

astro-ph.GA2019

The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties

A. Viitanen, V. Allevato, A. Finoguenov +5

We study the spatial clustering through the projected two-point correlation function of XMM-COSMOS Active Galactic Nuclei (AGNs) with known spectroscopic (spectrosco…

astro-ph.CO2019

Estimating the galaxy two-point correlation function using a split random catalog

E. Keihänen, H. Kurki-Suonio, V. Lindholm +13

The two-point correlation function of the galaxy distribution is a key cosmological observable that allows us to constrain the dynamical and geometrical state of our Universe. To m…