All Outputs (4)

Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8 < 𝑧 < 1.5 (2025)
Journal Article
Hewitt, G., Sarron, F., Balogh, M. L., Rudnick, G., Bahé, Y., Baxter, D. C., Castignani, G., Cerulo, P., Cooper, M. C., Demarco, R., Edward, A. H., Finn, R. A., Forrest, B., Muzzin, A., Nantais, J., Vulcani, B., Wilson, G., & Zaritsky, D. (2025). Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8 < 𝑧 < 1.5. Monthly Notices of the Royal Astronomical Society, https://doi.org/10.1093/mnras/staf932

High-redshift (𝑧 ∼ 1) galaxy clusters are the domain where environmental quenching mechanisms are expected to emerge as important factors in the evolution of the quiescent galaxy population. Uncovering these initially subtle effects requires explorin... Read More about Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8 < 𝑧 < 1.5.

Insights into environmental quenching at z ∼1: an enhancement of faint, low-mass passive galaxies in clusters (2025)
Journal Article
Gully, H., Hatch, N., Ahad, S. L., Bahé, Y., Balogh, M., Baxter, D. C., Cerulo, P., Cooper, M. C., Demarco, R., Forrest, B., Rescigno, U., Rudnick, G., Vulcani, B., & Wilson, G. (2025). Insights into environmental quenching at z ∼1: an enhancement of faint, low-mass passive galaxies in clusters. Monthly Notices of the Royal Astronomical Society, 539(4), 3058-3076. https://doi.org/10.1093/mnras/staf635

Understanding the processes that transform star-forming galaxies into quiescent ones is key to unravelling the role of environment in galaxy evolution. We present measurements of the luminosity functions (LFs) and stellar mass functions (SMFs) of pas... Read More about Insights into environmental quenching at z ∼1: an enhancement of faint, low-mass passive galaxies in clusters.

Assembly of the intracluster light in the Horizon-AGN simulation (2024)
Journal Article
Brown, H. J., Martin, G., Pearce, F. R., Hatch, N. A., Bahé, Y. M., & Dubois, Y. (2024). Assembly of the intracluster light in the Horizon-AGN simulation. Monthly Notices of the Royal Astronomical Society, 534(1), 431-443. https://doi.org/10.1093/mnras/stae2084

The diffuse stellar component of galaxy clusters made up of intergalactic stars is termed the intracluster light (ICL). Although there is a developing understanding of the mechanisms by which the ICL is formed, no strong consensus has yet been reache... Read More about Assembly of the intracluster light in the Horizon-AGN simulation.

The FLAMINGO project: Cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys (2023)
Journal Article
Schaye, J., Kugel, R., Schaller, M., Helly, J. C., Braspenning, J., Elbers, W., McCarthy, I. G., Van Daalen, M. P., Vandenbroucke, B., Frenk, C. S., Kwan, J., Salcido, J., Bahe, Y. M., Borrow, J., Chaikin, E., Hahn, O., Huško, F., Jenkins, A., Lacey, C. G., & Nobels, F. S. (2023). The FLAMINGO project: Cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys. Monthly Notices of the Royal Astronomical Society, 526(4), 4978-5020. https://doi.org/10.1093/mnras/stad2419

We introduce the Virgo Consortium's FLAMINGO suite of hydrodynamical simulations for cosmology and galaxy cluster physics. To ensure the simulations are sufficiently realistic for studies of large-scale structure, the subgrid prescriptions for stella... Read More about The FLAMINGO project: Cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys.