Outputs (2)

Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions (2023)
Journal Article
Brough, S., Ahad, S. L., Bahé, Y. M., Ellien, A., Gonzalez, A. H., Jiménez-Teja, Y., …Mihos, J. C. (2024). Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions. Monthly Notices of the Royal Astronomical Society, 528(1), 771-795. https://doi.org/10.1093/mnras/stad3810

Intracluster light (ICL) provides an important record of the interactions galaxy clusters have undergone. However, we are limited in our understanding by our measurement methods. To address this, we measure the fraction of cluster light that is held... Read More about Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions.

Star formation concentration as a tracer of environmental quenching in action: a study of the eagle and c-eagle simulations (2023)
Journal Article
Wang, D., Lagos, C. D. P., Croom, S. M., Wright, R. J., Bahé, Y. M., Bryant, J. J., …Vaughan, S. P. (2023). Star formation concentration as a tracer of environmental quenching in action: a study of the eagle and c-eagle simulations. Monthly Notices of the Royal Astronomical Society, 523(4), 6020-6040. https://doi.org/10.1093/mnras/stad1864

We study environmental quenching in the EAGLE/C-EAGLE cosmological hydrodynamic simulations over the last 11 Gyr (i.e. z = 0–2). The simulations are compared with observations from the SAMI Galaxy Survey at z = 0. We focus on satellite galaxies in ga... Read More about Star formation concentration as a tracer of environmental quenching in action: a study of the eagle and c-eagle simulations.