Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Star formation, Metallicity, and Redshift.
Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation
Inspiraling streams of enriched gas observed around a massive galaxy 11 billion years ago
FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations
Virialization of the Inner CGM in the FIRE Simulations and Implications for Galaxy Disks, Star Formation, and Feedback
Gas-phase metallicity gradients of TNG50 star-forming galaxies
The bursty origin of the Milky Way thick disc
No missing photons for reionization: moderate ionizing photon escape fractions from the FIRE-2 simulations
Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
The impact of AGN wind feedback in simulations of isolated galaxies with a multiphase ISM
On the dust temperatures of high-redshift galaxies
Dust attenuation, dust emission, and dust temperature in galaxies at z ≥ 5: a view from the FIRE-2 simulations
Radiative stellar feedback in galaxy formation: Methods and physics
Predictions for the spatial distribution of the dust continuum emission in $\boldsymbol {1\,\lt\, z\,\lt\, 5}$ star-forming galaxies
The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
Cosmic rays or turbulence can suppress cooling flows (where thermal heating or momentum injection fail)
FIRE-2 simulations: physics versus numerics in galaxy formation
Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions
The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
The physics of Lyman α escape from high-redshift galaxies
Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction and metal diffusion on sub-L* galaxy formation
Modelling chemical abundance distributions for dwarf galaxies in the Local Group: the impact of turbulent metal diffusion
Metal flows of the circumgalactic medium, and the metal budget in galactic haloes
The structure and dynamical evolution of the stellar disc of a simulated Milky Way-mass galaxy
Formation of globular cluster candidates in merging proto-galaxies at high redshift: a view from the FIRE cosmological simulations
Why do high-redshift galaxies show diverse gas-phase metallicity gradients?
Binary stars can provide the ‘missing photons’ needed for reionization
The origin and evolution of the galaxy mass–metallicity relation
The difficulty of getting high escape fractions of ionizing photons from high-redshift galaxies: a view from the FIRE cosmological simulations