I contribute to multiple international simulation and survey collaborations focused on galaxy formation and cosmology.
FLARES
The First Light And Reionisation Epoch Simulations
Show detailsHide details
FLARES is a suite of high-redshift zoom simulations designed to probe rare environments at high fidelity and large effective volume. I led the first release paper and several follow-up studies on environmental trends and passive populations.
Cosmology and Astrophysics with MachinE Learning Simulations
Show detailsHide details
CAMELS stands for Cosmology and Astrophysics with MachinE Learning Simulations, and aims at building bridges between cosmology and astrophysics through large suites of numerical simulations and machine learning. I ran the SWIFT-EAGLE simulation suite, generated synthetic photometric catalogues, and worked on generative and inference-oriented modelling workflows.
Euclid is a recently launched space observatory that will survey a third of the sky, with exciting possibilities in exploring the dark sector as well as galaxy evolution with uinprecedented numbers of sources. I am part of the Euclid Consortium, junior deputy lead of the galaxy and AGN evolution scientific working group, and co-lead the passive galaxy and gravitational wave simulations work packages.
The Learning the Universe collaboration develops scalable forward-modelling and simulation-based inference pipelines for cosmology and astrophysics. I have contributed to pipeline development and applications combining synthetic observables with inference.
The Gravitational Waves x Galaxy Catalogues collaboration
Show detailsHide details
GWCats brings together the gravitational-wave and galaxy-catalog communities. It is focused on building shared catalogue and analysis frameworks that support multi-messenger science.
Simba is a leading hydrodynamic galaxy-formation simulation suite used for a diverse range of studies. I have contributed to dust RT modelling of dusty star forming galaxies, orientation-dependent emission analyses, and related high-redshift investigations.