collaborators

5 papers

astro-ph.GA2026

The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies

Marcelo C. Vicentin, Michael A. Strauss, Laerte Sodré +3

We use the L-GALAXIES semi-analytic model to investigate the evolution of Brightest Cluster Galaxies (BCGs) found in clusters at . BCGs are typically located in the c…

astro-ph.GA2025

The role of mergers and rejuvenation in the buildup of the quiescent population at cosmic noon

Jimi Evan Harrold, Omar Almaini, Frazer R. Pearce +6

We investigate the quenching of galaxies using a mock observational lightcone generated from the Semi-Analytic Model (SAM) L-Galaxies, closely matched to observations from the UKID…

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

First joint absorption and T-based metallicity measured in a GRB host galaxy at using JWST/NIRSpec

Anne Inkenhaag, Patricia Schady, Phil Wiseman +20

We present the first gamma-ray burst (GRB) host galaxy with a measured absorption line and electron temperature (T) based metallicity, using the temperature sensitive [OIII]$λ…

astro-ph.GA2025

First IFU observations of two GRB host galaxies at cosmic noon with JWST/NIRSpec

B. Topçu, P. Schady, S. Wuyts +16

Long gamma-ray bursts (GRBs) serve as powerful probes of distant galaxies. Their luminous afterglow pinpoints galaxies independent of luminosity, in contrast to most flux-limited s…