Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Stellar, planetary, and galactic studies, and Astrophysics and Star Formation Studies.
Bursting at the seams: the star-forming main sequence and its scatter at <i>z</i> = 3–9 using NIRCam photometry from JADES
Connecting <i>JWST</i> discovered N/O-enhanced galaxies to globular clusters: evidence from chemical imprints
<i>In-situ</i> versus accreted Milky Way globular clusters: a new classification method and implications for cluster formation
Nitrogen enrichment and clustered star formation at the dawn of the Galaxy
Taking the Milky Way for a spin: disc formation in the <scp>artemis</scp> simulations
Spatial and orbital planes of the Milky Way satellites: unusual but consistent with ΛCDM
From dawn till disc: Milky Way’s turbulent youth revealed by the APOGEE+<i>Gaia</i> data
Excluding fuzzy dark matter with sizes and stellar kinematics of ultrafaint dwarf galaxies
<scp>grumpy</scp>: a simple framework for realistic forward modelling of dwarf galaxies
Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogues
Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
The mass and galaxy distribution around SZ-selected clusters
Thermal instability in the CGM of <i>L</i>⋆ galaxies: testing ‘precipitation’ models with the FIRE simulations
Milky Way Satellite Census. II. Galaxy–Halo Connection Constraints Including the Impact of the Large Magellanic Cloud
The three causes of low-mass assembly bias
The Sheet of Giants: Unusual properties of the Milky Way’s immediate neighbourhood
Measurement of the splashback feature around SZ-selected Galaxy clusters with DES, SPT, and ACT
Imprints of mass accretion history on the shape of the intracluster medium and the TX–M relation
How Galaxies Form Stars: The Connection between Local and Global Star Formation in Galaxy Simulations
The Splashback Feature around DES Galaxy Clusters: Galaxy Density and Weak Lensing Profiles
Enforcing the Courant–Friedrichs–Lewy condition in explicitly conservative local time stepping schemes
DES Y1 Results: validating cosmological parameter estimation using simulated Dark Energy Surveys
Cold fronts and shocks formed by gas streams in galaxy clusters
Umbrella sampling: a powerful method to sample tails of distributions
STAR CLUSTER FORMATION IN COSMOLOGICAL SIMULATIONS. I. PROPERTIES OF YOUNG CLUSTERS
The Physical Origin of Long Gas Depletion Times in Galaxies
The Halo Boundary of Galaxy Clusters in the SDSS
Quenching of satellite galaxies at the outskirts of galaxy clusters
Cosmology from cosmic shear with Dark Energy Survey Science Verification data
DETECTION OF THE SPLASHBACK RADIUS AND HALO ASSEMBLY BIAS OF MASSIVE GALAXY CLUSTERS
Investigating the physical origin of satellite planes
Modeling turbulent galaxy formation
Collaborative research: Exploring the impact of cosmic ray feedback on galaxy evolution
Collaborative Research: Modelling the Turbulent Galaxy Formation
NSF Astronomy & Astrophysics Postdoctoral Fellows 2014 Symposium
Collaborative Research: Towards Petascale Cosmological Simulations
COLLABORATIVE RESEARCH: New Frontiers in Galaxy Formation Modeling
COLLABORATIVE RESEARCH: Modeling formation of dwarf galaxies from the Cosmic Renaissance to the Present
CAREER: Simulations of Galaxy and Cluster Formation: The New Frontiers
High-Resolution Simulations of Galaxy and Cluster Formation: Towards a Self-Consistent Modelling of Stellar Feedback