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20222026
most citedEnrichment by Extragalactic First Stars in the Large Magellanic Cloud

22 citations · 58 across the 21 of their papers we have counts for

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9 papers · 1 filter

astro-ph.SR2026

The -Process Alliance: On J00101735, an Accreted, Chemically Unusual, Metal-poor Star with -process Enhancement

Zoe Hackshaw, Rana Ezzeddine, Shivani P. Shah +11

We present a detailed chemo-dynamical analysis of the chemically peculiar very metal-poor ([Fe/H]) Milky Way (MW) halo star, 2MASS J001017581735387 (hereafter J0…

astro-ph.SR2026

Payne4GAIN: NLTE Corrections for Red Giants in Milky Way Mapper using H-Band Neural Network Emulators

Pierre Thibodeaux, Alexander P. Ji, Nicholas Storm +12

The majority of spectroscopic surveys assume local thermodynamic equilibrium (LTE) during the modeling of stellar spectra. This assumption begins to break down for luminous stars,…

astro-ph.SR2026

The -Process Alliance: Actinide Abundances, Variation, and Evolution in Metal-Poor Stars

Shivani P. Shah, Rana Ezzeddine, Erika M. Holmbeck +11

The actinides, including thorium (Th), are the heaviest observable elements synthesized in the universe, holding clues to the extremes of the astrophysical and nuclear conditions o…

astro-ph.SR2026

Evaluating Classifications of Extremely Metal-poor Candidates Selected from Gaia XP Spectra

Riley Thai, Andrew R. Casey, Alexander Ji +2

Extremely metal-poor stars are intrinsically rare, but emerging methods exist to accurately classify them from all-sky Gaia XP low-resolution spectra. To assess their overall accur…

astro-ph.SR2025★ 2 cited

A nearly pristine star from the Large Magellanic Cloud

Alexander P. Ji, Vedant Chandra, Selenna Mejias-Torres +28

The first stars formed out of pristine gas, causing them to be so massive that none are expected to have survived until today. If their direct descendants were sufficiently low-mas…

astro-ph.SR2025★ 3 cited

The R-Process Alliance: Hunting for gold in the near-UV spectrum of 2MASS J05383296-5904280

Terese T. Hansen, Ian U. Roederer, Shivani P. Shah +10

Context. Over the past few years, the -Process Alliance (RPA) has successfully carried out a search for stars that are highly enhanced in elements produced via the rapid neutron…

astro-ph.SR2024★ 7 cited

LAMOST J1010+2358 is not a Pair-Instability Supernova Relic

Pierre N. Thibodeaux, Alexander P. Ji, William Cerny +2

The discovery of a star formed out of pair-instability supernova ejecta would have massive implications for the Population III star initial mass function and the existence of stars…

astro-ph.SR2024

The -Process Alliance: Detailed Composition of an -Process Enhanced Star with UV and Optical Spectroscopy

Shivani P. Shah, Rana Ezzeddine, Ian U. Roederer +8

We present a detailed chemical-abundance analysis of a highly -process enhanced (RPE) star, 2MASS J00512646-1053170, using high-resolution spectroscopic observations with $Hubbl…

astro-ph.SR2024

Spectacular nucleosynthesis from early massive stars

Alexander P. Ji, Sanjana Curtis, Nicholas Storm +39

Stars formed with initial mass over 50 Msun are very rare today, but they are thought to be more common in the early universe. The fates of those early, metal-poor, massive stars a…