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.
The DECam MAGIC Survey: Spectroscopic Follow-up of the Most Metal-poor Stars in the Distant Milky Way Halo<sup>*</sup>
Identifying Dwarfs of MC Analog GalaxiEs (ID-MAGE): The Search for Satellites around Low-mass Hosts
A dark siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and DELVE
A Search for Faint Resolved Galaxies Beyond the Milky Way in DES Year 6: A New Faint, Diffuse Dwarf Satellite of NGC 55
The Faint Satellite System of NGC 253: Insights into Low-density Environments and No Satellite Plane*
Gas and Star Formation in Satellites of Milky Way Analogs
All Puffed Up: Exploring Ultra-diffuse Galaxy Origins Through Galaxy Interactions
Reading between the (Spectral) Lines: Magellan/IMACS Spectroscopy of the Ultrafaint Dwarf Galaxies Eridanus IV and Centaurus I
Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus
Timing the r-process Enrichment of the Ultra-faint Dwarf Galaxy Reticulum II
Characterizing the intracluster light over the redshift range 0.2 &lt; <i>z</i> &lt; 0.8 in the DES-ACT overlap
Limit on Supernova Emission in the Brightest Gamma-Ray Burst, GRB 221009A
DELVE 6: An Ancient, Ultra-faint Star Cluster on the Outskirts of the Magellanic Clouds
Pavo: Discovery of a Star-forming Dwarf Galaxy Just Outside the Local Group*
Identification of Galaxy–Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
The quenched satellite population around Milky Way analogues
The DECam Local Volume Exploration Survey Data Release 2
Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 Mpc*
Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies*
Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies
Gas-rich, Field Ultra-diffuse Galaxies Host Few Gobular Clusters
Resolved Dwarf Galaxy Searches within ∼5 Mpc with the Vera Rubin Observatory and Subaru Hyper Suprime-Cam*
Very Large Telescope Spectroscopy of Ultra-faint Dwarf Galaxies. I. Boötes I, Leo IV, and Leo V
Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations
Evidence for Ultra-Diffuse Galaxy Formation Through Tidal Heating of Normal Dwarfs
The M101 Satellite Luminosity Function and the Halo–Halo Scatter among Local Volume Hosts