activity
20082023
most citedEvolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

312 citations · 5.2k across the 102 of their papers we have counts for

collaborators

99 papers

astro-ph.GA2023★ 2 cited

Star formation and AGN activity 500 Myr after the Big Bang: Insights from JWST

Jordan C. J. D'Silva, Simon P. Driver, Claudia D. P. Lagos +3

We consider the effect of including an active galactic nuclei (AGN) component when fitting spectral energy distributions of 109 spectroscopically confirmed gala…

astro-ph.GA2023★ 6 cited

Quenching massive galaxies across cosmic time with the semi-analytic model SHARK v2.0

Claudia D. P. Lagos, Matias Bravo, Rodrigo Tobar +7

We introduce version 2.0 of the SHARK semi-analytic model of galaxy formation after many improvements to the physics included. The most significant being: (i) a model describing th…

astro-ph.GA2023

VERTICO VII: Environmental quenching caused by suppression of molecular gas content and star formation efficiency in Virgo Cluster galaxies

Toby Brown, Ian D. Roberts, Mallory Thorp +20

We study how environment regulates the star formation cycle of 33 Virgo Cluster satellite galaxies on 720 parsec scales. We present the first resolved star-forming main sequence fo…

astro-ph.GA2023★ 123 cited

A massive galaxy that formed its stars at

Karl Glazebrook, Themiya Nanayakkara, Corentin Schreiber +15

The formation of galaxies by gradual hierarchical co-assembly of baryons and cold dark matter halos is a fundamental paradigm underpinning modern astrophysics and predicts a strong…

astro-ph.GA2023★ 2 cited

Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG

Jennifer A. Hardwick, Luca Cortese, Danail Obreschkow +4

We use the EAGLE (Evolution and Assembly of GaLaxies and their Environments) and IllustrisTNG (The Next Generation) cosmological simulations to investigate the properties of the ba…

astro-ph.GA2023★ 23 cited

GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years

Jordan C. J. D'Silva, Simon P. Driver, Claudia D. P. Lagos +11

We use the Galaxy and Mass Assembly (GAMA) and the Deep Extragalactic Visible Legacy Survey (DEVILS) observational data sets to calculate the cosmic star formation rate (SFR) and a…