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
Showing 2021Show all

7 papers · 1 filter

astro-ph.GA2021★ 68 cited

VERTICO: The Virgo Environment Traced In CO Survey

Toby Brown, Christine D. Wilson, Nikki Zabel +33

We present the Virgo Environment Traced in CO (VERTICO) survey, a new effort to map CO(), CO(), and CO() in 51 Virgo Cluster galaxies with the A…

astro-ph.GA2021★ 34 cited

The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics

Jesse van de Sande, Scott M. Croom, Joss Bland-Hawthorn +16

The kinematic morphology-density relation of galaxies is normally attributed to a changing distribution of galaxy stellar masses with the local environment. However, earlier studie…

astro-ph.GA2021★ 7 cited

The HI and stellar mass bivariate distribution of centrals and satellites for all, late- and early-type local galaxies

A. R. Calette, Vladimir Avila-Reese, Aldo Rodríguez-Puebla +2

We characterize the conditional distributions of the HI gas-to-stellar mass ratio, , given the stellar mass, , of local galaxies from $M_{\a…

astro-ph.GA2021★ 4 cited

The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies

Robert Mostoghiu, Alexander Knebe, Frazer R. Pearce +7

Using 324 numerically modelled galaxy clusters as provided by THE THREE HUNDRED project, we study the evolution of the kinematic properties of the stellar component of haloes on fi…

astro-ph.GA2021★ 48 cited

COALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16

S. Jin, H. Dannerbauer, B. Emonts +25

We report a detailed CO(1-0) survey of a galaxy protocluster field at , based on 475 hours of observations with the Australia Telescope Compact Array. We constructed a larg…

astro-ph.GA2021★ 25 cited

Unveiling the atomic hydrogen-halo mass relation via spectral stacking

Garima Chauhan, Claudia del P. Lagos, Adam R. H. Stevens +5

Measuring the HI-halo mass scaling relation (HIHM) is fundamental to understanding the role of HI in galaxy formation and its connection to structure formation. While direct measur…