Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Astronomy, Stars, Globular cluster, and Photometry (optics).
The JWST Resolved Stellar Populations Early Release Science Program. V. DOLPHOT Stellar Photometry for NIRCam and NIRISS
A JWST Project on 47 Tucanae. Overview, Photometry, and Early Spectroscopic Results of M Dwarfs and Observations of Brown Dwarfs*
Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
POSYDON: A General-purpose Population Synthesis Code with Detailed Binary-evolution Simulations
The JWST Resolved Stellar Populations Early Release Science Program. II. Survey Overview
The Hubble Space Telescope Survey of M31 Satellite Galaxies. II. The Star Formation Histories of Ultrafaint Dwarf Galaxies
oMEGACat. I. MUSE Spectroscopy of 300,000 Stars within the Half-light Radius of ω Centauri
Investigating the Lower Mass Gap with Low-mass X-Ray Binary Population Synthesis
A Black Hole Kicked at Birth: MAXI J1305-704
The Hubble Space Telescope Survey of M31 Satellite Galaxies. I. RR Lyrae–based Distances and Refined 3D Geometric Structure
The impact of mass-transfer physics on the observable properties of field binary black hole populations
Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
Erratum: “A Complete Census of Luminous Stellar Variability on Day to Decade Timescales” (2018, ApJ, 864, 111)
Helium Variation in Four Small Magellanic Cloud Globular Clusters
The Large-scale Structure of the Halo of the Andromeda Galaxy. II. Hierarchical Structure in the Pan-Andromeda Archaeological Survey
The GALAH survey: verifying abundance trends in the open cluster M67 using non-LTE modelling
Ruprecht 106: A Riddle, Wrapped in a Mystery, inside an Enigma<sup>∗</sup>
NGC 1866: First Spectroscopic Detection of Fast-rotating Stars in a Young LMC Cluster
The HST large programme on ω Centauri – I. Multiple stellar populations at the bottom of the main sequence probed in NIR–Optical
The GALAH survey: scientific motivation
STRÖMGREN SURVEY FOR ASTEROSEISMOLOGY AND GALACTIC ARCHAEOLOGY: LET THE SAGA BEGIN
The halo+cluster system of the Galactic globular cluster NGC 1851★
MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS
An age difference of two billion years between a metal-rich and a metal-poor globular cluster
ULTRA-DEEP<i>HUBBLE SPACE TELESCOPE</i>IMAGING OF THE SMALL MAGELLANIC CLOUD: THE INITIAL MASS FUNCTION OF STARS WITH<i>M</i>≲ 1<i>M</i><sub>☉</sub>
The stellar metallicity distribution of disc galaxies and bulges in cosmological simulations