activity
20242026
collaborators

6 papers

astro-ph.GA2026

Ruffled Feathers: Merger-driven galaxy size growth and structural transformation in EAGLE

Kai Wang, Carlton Baugh, Sownak Bose +9

Galaxy mergers drive both the size growth and the transformation from discs to spheroids, yet the prescriptions used to model these processes in semi-analytic frameworks have not b…

astro-ph.GA2026

Inflow-driven galaxy evolution - I. Revealing the physics of the fundamental metallicity relation

Kai Wang, Carlton Baugh, N. F. Boardman +11

We present a unified physical framework for the fundamental metallicity relation (FMR), based on the mass-continuity equations. The FMR is not merely the anti-correlation between s…

astro-ph.GA2026

Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array

Claudia del P. Lagos, Carlton M. Baugh, Connor Bottrell +11

Over the past decade, galaxy formation simulations have advanced dramatically, transforming our ability to model the interstellar medium (ISM) and predict galaxies' radio emission.…

astro-ph.GA2025

First Light And Reionisation Epoch Simulations (FLARES) XX: Comparing semi-analytic models at high-redshift

Louise T. C. Seeyave, Carlton M. Baugh, Angel Chandro-Gomez +13

We explore how the choice of galaxy formation model affects the predicted properties of high-redshift galaxies. Using the FLARES zoom resimulation strategy, we compare the EAGLE hy…

astro-ph.GA2025

The diverse star formation histories of early massive, quenched galaxies in modern galaxy formation simulations

Claudia del P. Lagos, Francesco Valentino, Ruby J. Wright +13

We present a comprehensive study of the star formation histories of massive-quenched galaxies at in 3 semi-analytic models (SHARK, GAEA, GALFORM) and 3 cosmological hydrodyna…

astro-ph.GA2024

A comparison of pre-existing CDM predictions with the abundance of {\it JWST} galaxies at high redshift

Shengdong Lu, Carlos S. Frenk, Sownak Bose +4

Observations with the {\it James Webb Space Telescope} have revealed a high abundance of bright galaxies at redshift, , which has been widely interpreted as conflictin…