activity
20092026
most citedA unified multi-wavelength model of galaxy formation

426 citations · 4.3k across the 76 of their papers we have counts for

collaborators

78 papers

astro-ph.GA2026

The Role of Environment in Shaping the Assembly Timelines of Massive Quiescent Galaxies at Cosmic Noon

Tianmu Gao, J. Trevor Mendel, Letizia Bugiani +10

JWST observations of massive quiescent galaxies (MQGs) at have revealed diverse star formation histories (SFHs). In this letter, we investigate whether these variations ar…

astro-ph.GA2026

Dust in the Average Galaxy: Attenuation, Emission, and Opacity from

Caitlin M. Casey, Hollis B. Akins, Andrew J. Battisti +43

We present constraints on the dust emission and attenuation properties of galaxies across 0<z<7 using JWST imaging from the COSMOS-Web Survey combined with deep FIR/(sub)millimeter…

astro-ph.GA2026

Unveiling the population of massive quenched galaxies at in the COLIBRE simulations - II. The role of AGN feedback and environment on their emergence

Ángel Chandro-Gómez, Claudia del P. Lagos, Chris Power +16

Early () Massive (), Quenched Galaxies (MQGs) challenge current galaxy formation models. In this series, we study these…

astro-ph.GA2026

Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since

Yunchong Zhang, Zhiyuan Ji, Rachel Bezanson +17

Massive quiescent galaxies have been identified out to in early JWST data in a substantial excess ( at ) of number densities from most theoretical…

astro-ph.GA2026

FEASTS and MHONGOOSE: HI Column Density Distribution at for

Jing Wang, Xuchen Lin, Ze-Zhong Liang +24

We present the first HI column density distribution function, , extending down to . This was derived from high-s…

astro-ph.GA2026★ 2 cited

The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0

Megan K. Oxland, Matías Bravo, Laura C. Parker +1

Observational studies have made substantial progress in characterizing quenching as a function of stellar mass and environment, but they are often limited in their ability to const…

astro-ph.GA2026

The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory

Jordan C. J. D'Silva, Simon P. Driver, Aaron S. G. Robotham +5

We compute the cosmic stellar, dust and neutral gas mass history at using ProSpect spectral energy distribution modelling of galaxies in the Gal…

astro-ph.GA2025

Unveiling the population of massive quenched galaxies at in the COLIBRE simulations - I. Galaxy demographics

Ángel Chandro-Gómez, Claudia del P. Lagos, Chris Power +14

The James Webb Space Telescope has uncovered a substantial population of Massive (), Quenched Galaxies (MQGs) in the early Universe ($z \ge…

astro-ph.GA2025★ 2 cited

Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations

Claudia del P. Lagos, Joop Schaye, Matthieu Schaller +16

We investigate the correlation between star formation rate (SFR) surface density and gas surface density (known as the Kennicutt-Schmidt, KS, relation) at kiloparsec (kpc) scales a…

astro-ph.GA2025★ 1 cited

VENUS: A Strongly Lensed Clumpy Galaxy at behind the Galaxy Cluster MACS J0257.1-2325

Minami Nakane, Vasily Kokorev, Seiji Fujimoto +75

We present the discovery of a strongly lensed galaxy at , dubbed the ``Misty Moons'', identified in the JWST Treasury Survey, Vast Exploration for Nascent, Unexplored S…

astro-ph.GA2025★ 4 cited

A census of quiescent galaxies across with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe

Tiancheng Yang, Tao Wang, Ke Xu +12

Recent JWST observations have revealed a large population of quiescent galaxies (QGs) at high redshift (), challenging current models of early galaxy formation and quen…

astro-ph.GA2024★ 3 cited

The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies

Katy L. Proctor, Aaron D. Ludlow, Claudia del P. Lagos +1

Stellar haloes form through the disruption of satellite galaxies over time, making them a promising observable for constraining galaxy merger histories. We use a dynamical decompos…

astro-ph.GA2024

A Comparative Study of the Ground State Transitions of CO and [C I] as Molecular Gas Tracers at High Redshift

Marta Frias Castillo, Matus Rybak, Jacqueline A. Hodge +22

The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM)…

astro-ph.GA2023

The distribution of stellar orbits in Eagle galaxies -- the effect of mergers, gas accretion, and secular evolution

Giulia Santucci, Claudia Del P. Lagos, Katherine E. Harborne +9

The merger history of a galaxy is thought to be one of the major factors determining its internal dynamics, with galaxies having undergone different types or mergers (e.g. dry, min…

astro-ph.GA2023

SimSpin v2.6.0 -- Constructing synthetic spectral IFU cubes for comparison with observational surveys

K. E. Harborne, A. Serene, E. J. A. Davies +10

In this work, we present a methodology and a corresponding code-base for constructing mock integral field spectrograph (IFS) observations of simulated galaxies in a consistent and…

astro-ph.GA2023★ 1 cited

Identifying the discs, bulges, and intra-halo light of simulated galaxies through structural decomposition

Katy L. Proctor, Claudia del P. Lagos, Aaron D. Ludlow +1

We perform a structural decomposition of galaxies identified in three cosmological hydrodynamical simulations by applying Gaussian Mixture Models (GMMs) to the kinematics of their…

astro-ph.GA2023★ 1 cited

Resolving cosmic star formation histories of present-day bulges, disks, and spheroids with ProFuse

Sabine Bellstedt, Aaron S. G. Robotham, Simon P. Driver +3

We present the first look at star formation histories of galaxy components using ProFuse, a new technique to model the 2D distribution of light across multiple wavelengths using si…

astro-ph.GA2023★ 4 cited

Unbiased surveys of dust-enshrouded galaxies using ALMA

K. Kohno, S. Fujimoto, A. Tsujita +43

The ALMA lensing cluster survey (ALCS) is a 96-hr large program dedicated to uncovering and characterizing intrinsically faint continuum sources and line emitters with the assistan…

astro-ph.CO2023★ 12 cited

Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass

Ajay Dev, Simon P. Driver, Martin Meyer +11

We determine the atomic hydrogen (HI) to halo mass relation (HIHM) using Arecibo Legacy Fast ALFA survey HI data at the location of optically selected groups from the Galaxy and Ma…

astro-ph.CO2023★ 1 cited

The Spitzer Extragalactic Representative Volume Survey and DeepDrill extension: clustering of near-infrared galaxies

Eelco van Kampen, Mark Lacy, Duncan Farrah +7

We have measured the angular auto-correlation function of near-infrared galaxies in SERVS+DeepDrill, the Spitzer Extragalactic Representative Volume Survey and its follow-up survey…

astro-ph.GA2023★ 1 cited

Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C and SAMI surveys: direct evidence for merger-driven growth over the last 7 Gy

Francesco D'Eugenio, Arjen van der Wel, Joanna M. Piotrowska +37

We present the first study of spatially integrated higher-order stellar kinematics over cosmic time. We use deep rest-frame optical spectroscopy of quiescent galaxies at redshifts…

astro-ph.GA2023

Different higher-order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI and LEGA-C surveys

Francesco D'Eugenio, Arjen van der Wel, Caro Derkenne +38

We present the first statistical study of spatially integrated non-Gaussian stellar kinematics spanning 7 Gyr in cosmic time. We use deep, rest-frame optical spectroscopy of massiv…

astro-ph.GA2023★ 9 cited

Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0

Rongjun Huang, Andrew J. Battisti, Kathryn Grasha +4

Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass (), evolves…

astro-ph.GA2023★ 16 cited

The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux

Scott A. Tompkins, Simon P. Driver, Aaron S. G. Robotham +4

We present a revised measurement of the extra-galactic background light (EBL) at radio frequencies based on a near complete compendium of radio source counts. We present the radio-…