Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Astronomy, Dwarf galaxy, and Star formation.
Primordial rotating disk composed of at least 15 dense star-forming clumps at cosmic dawn
COSMOS-Web: Intrinsically Luminous z ≳ 10 Galaxy Candidates Test Early Stellar Mass Assembly
Early galaxies and early dark energy: a unified solution to the hubble tension and puzzles of massive bright galaxies revealed by <i>JWST</i>
The JWST Resolved Stellar Populations Early Release Science Program. V. DOLPHOT Stellar Photometry for NIRCam and NIRISS
Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4–8 from CEERS
Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
The JWST Resolved Stellar Populations Early Release Science Program. IV. The Star Formation History of the Local Group Galaxy WLM
Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation
The impact of UV variability on the abundance of bright galaxies at <i>z</i> ≥ 9
What causes the formation of discs and end of bursty star formation?
The JWST Resolved Stellar Populations Early Release Science Program. II. Survey Overview
Cosmological structure formation and soliton phase transition in fuzzy dark matter with axion self-interactions
The Hubble Space Telescope Survey of M31 Satellite Galaxies. II. The Star Formation Histories of Ultrafaint Dwarf Galaxies
Metallicity Distribution Functions of 13 Ultra-faint Dwarf Galaxy Candidates from Hubble Space Telescope Narrowband Imaging
Orientations of Dark Matter Halos in FIRE-2 Milky Way–mass Galaxies
FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations
Hot-mode accretion and the physics of thin-disc galaxy formation
The Hubble Space Telescope Survey of M31 Satellite Galaxies. I. RR Lyrae–based Distances and Refined 3D Geometric Structure
Galaxies lacking dark matter produced by close encounters in a cosmological simulation
Extinguishing the FIRE: environmental quenching of satellite galaxies around Milky Way-mass hosts in simulations
Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes
Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
The formation times and building blocks of Milky Way-mass galaxies in the FIRE simulations
Growing Pains: The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
arXiv (Cornell University) 2020cited by 6position: middle
The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations
Be it therefore resolved: cosmological simulations of dwarf galaxies with 30 solar mass resolution
First Star-Forming Structures in Fuzzy Cosmic Filaments
Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment
A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations