activity
20172026
most citedThe FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys

258 citations · 550 across the 40 of their papers we have counts for

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41 papers · 1 filter

astro-ph.GA2026

Galactic Morpholography: Linking present-day galaxy compactness to assembly history and relic formation in the COLIBRE simulations

Maximilian Zemsch, Claudia D. P. Lagos, Chiara Spiniello +11

Compactness is widely used to identify candidate relic galaxies, the largely untouched survivors of the first compact massive galaxies. Yet relicness is an evolutionary rather than…

astro-ph.GA2026

Atomic hydrogen in galaxies in the COLIBRE simulations

Kyle A. Oman, Ruby J. Wright, Andrea Gebek +12

We present an overview of the properties of atomic hydrogen (HI) in galaxies at redshift in the COLIBRE cosmological galaxy formation simulations. COLIBRE directly simulates…

astro-ph.GA2026

Mergers may not be the main channel for galaxy stellar mass growth at redshift : Predictions from cosmological hierarchical models and simulations

Hao Fu, Mohammadreza Ayromlou, Francesco Shankar +13

Mergers are a crucial channel of galaxy growth, but their role relative to star formation remains uncertain at high redshift. Here we investigate merger rates and merger-driven ste…

astro-ph.GA2026

Clustering-based halo mass assignment for high-redshift galaxies: method, validation, and application to JWST

Seunghwan Lim, Sandro Tacchella, Sara Saleh +7

We present a clustering-based method for inferring halo masses of high-redshift galaxies, validated using the COLIBRE simulations combined with the HOMA empirical model, which assu…

astro-ph.GA2026

The atomic multiphase interstellar medium of galaxies in the COLIBRE simulations

Moa Huppenkothen, Sylvia Ploeckinger, Joop Schaye +7

We analyse the neutral ISM of galaxies at redshift z=0 in the COLIBRE hydrodynamical simulations and investigate the conditions under which these two gas phases coexist in a narrow…

astro-ph.GA2026

The origin of the stellar mass-size relation of satellite galaxies in the COLIBRE simulations

Bruno M. Celiz, Julio F. Navarro, Joop Schaye +9

We study the stellar mass-size relation of satellite galaxies in the COLIBRE suite of cosmological hydrodynamical simulations. Satellites deviate from the relation that holds for c…

astro-ph.GA2026

The descendants of JWST galaxies in the COLIBRE simulations

Xu Zhao, Carlos S. Frenk, Andrew Pontzen +9

Recent observations with JWST have revealed a population of UV-bright galaxies at . This discovery naturally raises the question: what do such early galaxies evolve in…

astro-ph.GA2026

The progenitors of JWST galaxies in the COLIBRE simulations

Evgenii Chaikin, Andrew Pontzen, Carlos S. Frenk +4

JWST has revealed a large population of luminous galaxies () at redshifts , widely interpreted as posing a challenge to models of galaxy forma…

astro-ph.GA2026

The effect of galaxy interactions on star formation rates in the COLIBRE simulations

Quinten W. E. van Zegveld, Evgenii Chaikin, Joop Schaye +8

Observations and theory indicate that galaxy interactions enhance star formation rates (SFRs). However, the degree of enhancement and its dependence on the properties of the intera…

astro-ph.GA2026

The influence of feedback on the baryonic content of haloes in the COLIBRE simulations

Jonathan J. Davies, Joop Schaye, Filip Huško +7

We present predictions for the relation between the halo gas mass fraction and halo mass, , from the COLIBRE cosmological simulations of galaxy formation…

astro-ph.GA2026

The evolution of galaxy dust scaling relations in the COLIBRE simulations

Aswin P. Vijayan, James W. Trayford, Joop Schaye +11

We present dust scaling relations across cosmic time () for galaxies in the COLIBRE cosmological simulations. COLIBRE self-consistently tracks dust production, grow…

astro-ph.GA2026

Cosmological simulations of the high-redshift galaxy population adopting a variable stellar initial mass function

Anna Durrant, Robert A. Crain, Cedric G. Lacey +15

JWST surveys reveal a greater space density of high-redshift UV-bright galaxies than predicted by conventional galaxy formation models. We present results from a cMpc cosmo…

astro-ph.GA2026

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations

Andrea Gebek, Maarten Baes, Nick Andreadis +16

Context. Three-dimensional dust radiative transfer provides a powerful framework to connect cosmological galaxy simulations to multiwavelength observations. Until recently, in larg…

astro-ph.GA2026

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium

Jemima M. Briggs, Azadeh Fattahi, Robert A. Crain +7

We introduce a suite of LambdaCDM cosmological, hydrodynamical simulations that track the evolution of a large population of dwarf galaxies. The suite comprises zoom-in simulations…

astro-ph.GA2026

The evolution of the galaxy gas-phase mass-metallicity relation from to in the COLIBRE cosmological simulations

Piyush Sharda, Joop Schaye, Robert J. McGibbon +8

We present the evolution of the galaxy gas-phase mass-metallicity relation (MZR) from to in the COLIBRE cosmological hydrodynamical simulations. Amongst other novel fe…

astro-ph.GA2026

The galaxy ultraviolet luminosity function from to in the COLIBRE simulations

Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey +17

JWST has enabled the detection of galaxies in the earliest stages of cosmic history. We compare the ultraviolet luminosity functions (UVLFs) at redshifts predicted by a se…

astro-ph.GA2026

Galaxy luminosity functions from far-UV to submillimetre at in the COLIBRE simulations

Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey +15

We present predictions from the COLIBRE cosmological hydrodynamical simulations of galaxy formation for the present-day galaxy luminosity functions (LFs) at wavelengths ranging fro…

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

The morphologies of present-day galaxies in the COLIBRE simulations

Victor J. Forouhar Moreno, Joop Schaye, Matthieu Schaller +9

The diversity of galaxy morphologies and their relations with galaxy and halo properties is fundamental to understanding galaxy formation. Cosmological simulations of representativ…

astro-ph.GA2026

The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE

Feihong He, Jiaxin Han, Joop Schaye +12

We investigate the co-evolution of the stellar and dark matter mass of satellite galaxies using the COLIBRE cosmological hydrodynamical simulations with subhaloes resolved by the h…

astro-ph.GA2026

A subgrid model for chemical enrichment in cosmological simulations

Camila A. Correa, Joop Schaye, Matthieu Schaller +6

We present the modules for stellar nucleosynthesis, stellar mass loss, and turbulent diffusion of the new COLIBRE subgrid model for cosmological hydrodynamical simulations of galax…

astro-ph.GA2026

Simulating AGN wind feedback with variable feedback efficiencies in idealised disc galaxies

Jinning Liang, Cedric G. Lacey, Filip Huško +2

Active Galactic Nucleus (AGN) feedback plays a critical role in galaxy formation and evolution. AGN-driven winds can significantly influence their host galaxies, although the detai…

astro-ph.GA2026★ 2 cited

The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations

Aaron D. Ludlow, Katy L. Proctor, Joop Schaye +12

We analyse the sizes and specific angular momentum content of galaxies in the Colibre cosmological hydrodynamical simulations spanning two orders of magnitude in mass resolution. W…

astro-ph.GA2026

The importance of super-Eddington black hole accretion for the emergence of massive quiescent galaxies at high redshift

Evgenii Chaikin, Joop Schaye, Filip Huško +3

Recent JWST observations indicate that massive quiescent galaxies (stellar mass ) at high redshift () are more abundant than pred…