BENITEZ LLAMBAY ALEJANDRO
- U02, Floor: 2, Room: 2009
Biography
Dr Benitez-Llambay is an Assistant Professor in the Physics Department at the University of Milano-Bicocca in Milan, Italy. His research intersects numerical cosmology, galaxy formation at the smallest scales, and 21 cm radio observations. Before arriving in Milan, he served as an Assistant Professor at the Astronomical Observatory of Córdoba, Argentina, and conducted research at the University of Victoria, Canada, and the Institute for Computational Cosmology in Durham, UK.
He tackles research challenges using advanced computational methods and large-scale cosmological simulations. He also develops high-performance software for creating and analyzing these datasets.
Additionally, Dr Benitez-Llambay is involved in major international collaborations focused on producing advanced hydrodynamical numerical models of galaxy formation within a cosmological context and exploring cosmological probes at the smallest scales using cutting-edge ground and space-based facilities.
Publications
Huško, F., Lacey, C., Schaye, J., Schaller, M., Chaikin, E., Ploeckinger, S., et al. (2026). A hybrid active galactic nucleus feedback model with spinning black holes, winds and jets. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 547(2), 1-46 [10.1093/mnras/stag324]. Detail
Benitez-Llambay, A., Ploeckinger, S., Schaye, J., Richings, A., Chaikin, E., Schaller, M., et al. (2026). Non-explosive pre-supernova feedback in the colibre model of galaxy formation. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 546(4), 1-27 [10.1093/mnras/stag268]. Detail
Chaikin, E., Schaye, J., Schaller, M., Ploeckinger, S., Benítez-Llambay, A., Frenk, C., et al. (2026). The evolution of the galaxy stellar mass function and star formation rates in thecolibresimulations from redshift 17 to 0. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 548(4 (June 2026)) [10.1093/mnras/stag740]. Detail
Wang, K., Schaye, J., Benítez-Llambay, A., Chaikin, E., Carlos, S., Huško, F., et al. (2026). Gravitational potential drives the concentration dependence of the stellar mass–halo mass relation. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 546(2) [10.1093/mnras/stag110]. Detail
Lagos, C., Schaye, J., Schaller, M., Obreschkow, D., Bahé, Y., Benítez-Llambay, A., et al. (2026). Kennicutt–Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 549(2), 1-28 [10.1093/mnras/stag947]. Detail
Research projects
Awards
Research and teaching assignments
- Ricercatore/Ricercatrice universitario a t.d. - Università degli Studi di MILANO-BICOCCA, 2024 - 2027