Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, and Astrophysics and Star Formation Studies.
Effect of gas accretion on α-element bimodality in Milky Way-mass galaxies in the FIRE-2 simulations
Bar fraction and its dependence on host galaxy properties in the local Universe
Automating galaxy morphology classification using <i>k</i>-nearest neighbours and non-parametric statistics
First resolved stellar halo kinematics of a Milky Way-mass galaxy outside the Local Group: The flat counter-rotating halo in NGC 4945
Exploring the Diversity of Faint Satellites in the M81 Group
The Observable Properties of Galaxy Accretion Events in Milky Way–like Galaxies in the FIRE-2 Cosmological Simulations
Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite
Orientations of Dark Matter Halos in FIRE-2 Milky Way–mass Galaxies
The imprint of bursty star formation on alpha-element abundance patterns in Milky Way-like galaxies
3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations
Ultrafaint Dwarf Galaxy Candidates in the M81 Group: Signatures of Group Accretion
Globular Cluster Intrinsic Iron Abundance Spreads. II. Protocluster Metallicities and the Age–Metallicity Relations of Milky Way Progenitors
New globular cluster candidates in the M81 group
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
The Galaxy Progenitors of Stellar Streams around Milky Way–mass Galaxies in the FIRE Cosmological Simulations
The formation times and building blocks of Milky Way-mass galaxies in the FIRE simulations
Is NGC 300 a pure exponential disk galaxy?
Growing Pains: The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
arXiv (Cornell University) 2020cited by 6position: middle
Tracing the anemic stellar halo of M 101
A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
Globular Cluster Intrinsic Iron Abundance Spreads. I. Catalog
A Model for Clumpy Self-enrichment in Globular Clusters
Galaxies Grow Their Bulges and Black Holes in Diverse Ways
D1005+68: A New Faint Dwarf Galaxy in the M81 Group
Haloes at the ragged edge: the importance of the splashback radius
Decoding Galactic Merger Histories
HI4PI: a full-sky H i survey based on EBHIS and GASS
Diverse stellar haloes in nearby Milky Way mass disc galaxies