Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Stars, Metallicity, Galaxy, and Dwarf galaxy.
Discovery of an [Fe/H] ∼ −4.8 Star in Gaia XP Spectra<sup>*</sup>
Early <i>r</i>-process Enrichment and Hierarchical Assembly Across the Sagittarius Dwarf Galaxy*
The dark matter profile of the Milky Way inferred from its circular velocity curve
The black hole low-mass X-ray binary V404 Cygni is part of a wide triple
Enrichment by extragalactic first stars in the Large Magellanic Cloud
The <i>R</i>-Process Alliance: detailed chemical composition of an <i>r</i>-process enhanced star with UV and optical spectroscopy
Signatures of Tidal Disruption of the Hercules Ultrafaint Dwarf Galaxy*
Element abundance patterns in stars indicate fission of nuclei heavier than uranium
Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II*
Detailed Chemical Abundances of Stars in the Outskirts of the Tucana II Ultrafaint Dwarf Galaxy*
Timing the r-process Enrichment of the Ultra-faint Dwarf Galaxy Reticulum II
The Atari Disk, a Metal-poor Stellar Population in the Disk System of the Milky Way
Horizons: nuclear astrophysics in the 2020s and beyond
The chemical abundance pattern of the extremely metal-poor thin disc star 2MASS J1808−5104 and its origins
Magellan/IMACS spectroscopy of Grus I: A low metallicity ultra-faint dwarf galaxy
Possibilities and Limitations of Kinematically Identifying Stars from Accreted Ultra-faint Dwarf Galaxies
An extended halo around an ancient dwarf galaxy
r-Process elements from magnetorotational hypernovae
Exploring the Galaxy’s halo and very metal-weak thick disc with <i>SkyMapper</i> and <i>Gaia</i> DR2
Chemical Abundances in the Ultra-faint Dwarf Galaxies Grus I and Triangulum II: Neutron-capture Elements as a Defining Feature of the Faintest Dwarfs*
The lowest detected stellar Fe abundance: the halo star SMSS J160540.18−144323.1
Evidence for an Aspherical Population III Supernova Explosion Inferred from the Hyper-metal-poor Star HE 1327–2326<sup>∗</sup>
The SkyMapper DR1.1 search for extremely metal-poor stars
From Nuclei to the Cosmos: Tracing Heavy-Element Production with the Oldest Stars
The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo
The R-Process Alliance: A Comprehensive Abundance Analysis of HD 222925, a Metal-poor Star with an Extreme R-process Enhancement of [Eu/H] = −0.14*
Chemical Abundances of New Member Stars in the Tucana II Dwarf Galaxy<sup>∗</sup>
The predicted luminous satellite populations around SMC- and LMC-mass galaxies – a missing satellite problem around the LMC?
Predicting the locations of possible long-lived low-mass first stars: importance of satellite dwarf galaxies
BRIGHT METAL-POOR STARS FROM THE HAMBURG/ESO SURVEY. II. A CHEMODYNAMICAL ANALYSIS