activity
20142026
most citedBaryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids

201 citations · 1.9k across the 69 of their papers we have counts for

collaborators
Showing 2020Show all

9 papers · 1 filter

astro-ph.GA2020★ 28 cited

The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies

Facundo Rodriguez, Antonio D. Montero-Dorta, Raul E. Angulo +2

In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez \& Merchán in order to determine t…

astro-ph.HE2020★ 176 cited

The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution

Filippo Santoliquido, Michela Mapelli, Nicola Giacobbo +2

We evaluate the redshift distribution of binary black hole (BBH), black hole - neutron star binary (BHNS) and binary neutron star (BNS) mergers, exploring the main sources of uncer…

astro-ph.CO2020★ 15 cited

On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias

Antonio D. Montero-Dorta, M. Celeste Artale, L. Raul Abramo +1

We explore the potential of the kinetic Sunyaev-Zel'dovich (kSZ) effect as the cornerstone of a future observational probe for halo spin bias, the secondary dependence of halo clus…

astro-ph.GA2020★ 25 cited

Baryons Shaping Dark Matter Haloes

P. Cataldi, S. Pedrosa, P. Tissera +1

In this work we aim at investigating the effects of baryons on the dark matter (DM) haloes structure, focusing on the correlation between the presence and importance of stellar dis…

astro-ph.HE2020★ 57 cited

Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters

Michela Mapelli, Filippo Santoliquido, Yann Bouffanais +3

Hierarchical mergers are one of the distinctive signatures of binary black hole (BBH) formation through dynamical evolution. Here, we present a fast semi-analytic approach to simul…

astro-ph.CO2020★ 31 cited

The physical origins of low-mass spin bias

Beatriz Tucci, Antonio D. Montero-Dorta, L. Raul Abramo +2

At , higher-spin haloes with masses above have a higher bias than lower-spin haloes of the same mass. However, this…

astro-ph.CO2020★ 41 cited

Gravitational Wave mergers as tracers of Large Scale Structures

S. Libanore, M. C. Artale, D. Karagiannis +6

Clustering measurements of Gravitational Wave (GW) mergers in Luminosity Distance Space can be used in the future as a powerful tool for Cosmology. We consider tomographic measurem…

astro-ph.GA2020★ 28 cited

An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events

M. Celeste Artale, Yann Bouffanais, Michela Mapelli +5

We investigate the properties of the host galaxies of compact binary mergers across cosmic time. To this end, we combine population synthesis simulations together with galaxy catal…

astro-ph.GA2020★ 49 cited

The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300

Antonio D. Montero-Dorta, M. Celeste Artale, L. Raul Abramo +6

We use the improved IllustrisTNG300 magneto-hydrodynamical cosmological simulation to revisit the effect that secondary halo bias has on the clustering of the central galaxy popula…