activity
20052026
most citedNucleosynthetic signatures of the first stars

566 citations · 13.8k across the 201 of their papers we have counts for

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93 papers · 1 filter

astro-ph.GA2026

Chemo-dynamical Analysis of a CNO-Enhanced Ultra Metal-poor Star (): Insights into Early Enrichment by Faint Population III Supernova

Guilherme Limberg, Vinicius M. Placco, Alexander P. Ji +10

We report an independent identification of the ultra metal-poor (UMP) star () DR3 $\texttt{source_id}$ 4795913112968206720 (GDR3_479591) in the miss…

astro-ph.GA2026

Carbon Abundances in Metal-Poor Stars Reveal Distinct Galaxy and Star Formation Pathways in the Early Universe

Alexander Yelland, Anna Frebel, Xiaowei Ou +2

Carbon-enhanced metal-poor (CEMP; with and ) stars preserve information about early chemical enrichment, low-mass star formation, and th…

astro-ph.GA2026

The Metallicity Distribution of the Ultra-Faint Dwarf Galaxy Segue 1

Daisy Bissonette, Alexander P. Ji, Joshua D. Simon +6

Ultra-faint dwarf galaxies (UFDs; stellar masses ) offer unique insights into early chemical evolution in low-mass systems. However, interpreting their metalli…

astro-ph.GA2026

The -Process Alliance: The -Process Enhancement of Stars from Chemodynamically Tagged Groups in the Milky Way Halo

Jessica Merritt Agnos, Charli M. Sakari, Pedro Silva +9

As part of the ongoing work of the -Process Alliance (RPA), detailed abundance measurements of 29 heavy elements in three metal-poor stars, 2MASS J145929813852558, 2MASS J194…

astro-ph.GA2025★ 1 cited

Aeos is Mixing it Up: The (In)homogeneity of Metal Mixing Following Population III Star Formation

Jennifer Mead, Kaley Brauer, Greg L. Bryan +7

Stellar surface abundances are records of the state of the gas from which stars formed, and thus trace how individual elements have mixed into the surrounding medium following thei…

astro-ph.GA2025★ 13 cited

Discovery of an Star in XP Spectra

Guilherme Limberg, Vinicius M. Placco, Alexander P. Ji +5

We report on the discovery of GDR3_526285 ( DR3 Source ID 5262850721755411072), a star with and one of the lowest metal ($\text{atomic number} >…

astro-ph.GA2025★ 3 cited

A Bimodal Metallicity Distribution Function in the Ultra-Faint Dwarf Galaxy Reticulum II

Alice M. Luna, Alexander P. Ji, Anirudh Chiti +6

Star formation in ultra-faint dwarf galaxies (UFDs, ) is suppressed by reionization, but may not be completely quenched. The metallicity distribution function (MD…

astro-ph.GA2025★ 1 cited

Decoding the Galactic Twirl: The Downfall of Milky Way-mass Galaxies Rotation Curves in the FIRE Simulations

Xiaowei Ou, Lina Necib, Andrew Wetzel +3

Recent measurements of the Milky Way rotation curve found a sharp decline at around - kpc from the center of the Galaxy, suggesting that the Galactic dark matter halo is mu…

astro-ph.GA2025★ 2 cited

Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations

Kaley Brauer, Jennifer Mead, John H. Wise +7

We explore the effect of variations in the Population III (Pop III) initial mass function (IMF) and star-by-star feedback on early galaxy formation and evolution using the Aeos sim…

astro-ph.GA2025

Early r-process Enrichment and Hierarchical Assembly Across the Sagittarius Dwarf Galaxy

Xiaowei Ou, Alexander Yelland, Anirudh Chiti +3

Dwarf galaxies like Sagittarius (Sgr) provide a unique window into the early stages of galactic chemical evolution, particularly through their metal-poor stars. By studying the che…

astro-ph.GA2025★ 3 cited

GLIMPSE: An ultra-faint 10 Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at

Seiji Fujimoto, Rohan P. Naidu, John Chisholm +32

Detecting the first generation of stars, Population III (PopIII), has been a long-standing goal in astrophysics, yet they remain elusive even in the JWST era. Here we present a nov…

astro-ph.GA2024★ 1 cited

Metal-Poor Stars in the Milky Way System

Anna Frebel

Ancient, long-lived stars remain present in all components of our home galaxy, the Milky Way. Born a few hundred million after the Big Bang and during a time that marked the very b…

astro-ph.GA2024★ 7 cited

Aeos: Transport of Metals from Minihalos following Population III Stellar Feedback

Jennifer Mead, Kaley Brauer, Greg L. Bryan +7

We investigate how stellar feedback from the first stars (Population III) distributes metals through the interstellar and intergalactic medium using the star-by-star cosmological h…

astro-ph.GA2024★ 6 cited

All the Little Things in Abell 2744: 1000 Gravitationally Lensed Dwarf Galaxies at from JWST NIRCam Grism Spectroscopy

Rohan P. Naidu, Jorryt Matthee, Ivan Kramarenko +31

Dwarf galaxies hold the key to crucial frontiers of astrophysics, however, their faintness renders spectroscopy challenging. Here we present the JWST Cycle 2 survey, All the Little…

astro-ph.GA2024★ 1 cited

AEOS: Star-by-Star Cosmological Simulations of Early Chemical Enrichment and Galaxy Formation

Kaley Brauer, Andrew Emerick, Jennifer Mead +7

The AEOS project introduces a series of high-resolution cosmological simulations that model star-by-star chemical enrichment and galaxy formation in the early Universe, achieving 1…

astro-ph.GA2024

The -Process Alliance: Enrichment of -process Elements in a Simulated Milky Way-like Galaxy

Yutaka Hirai, Timothy C. Beers, Young Sun Lee +11

We study the formation of stars with varying amounts of heavy elements synthesized by the rapid neutron-capture process (-process) based on our detailed cosmological zoom-in sim…

astro-ph.GA2024★ 6 cited

The oldest stars with low neutron-capture element abundances and origins in ancient dwarf galaxies

Hillary Diane Andales, Ananda Santos Figueiredo, Casey Gordon Fienberg +2

We present a detailed chemical abundance and kinematic analysis of six extremely metal-poor ( [Fe/H] 2.9) halo stars with very low neutron-capture abundances ([Sr…

astro-ph.GA2024

The Rise of the -Process in the Gaia-Sausage/Enceladus Dwarf Galaxy

Xiaowei Ou, Alexander P. Ji, Anna Frebel +2

Neutron star mergers (NSMs) produce copious amounts of heavy r-process elements after a time delayed inspiral process. Once NSMs are present in a galaxy, r-process elements, such a…

astro-ph.GA2024

Signatures of tidal disruption of the Hercules ultra-faint dwarf galaxy

Xiaowei Ou, Anirudh Chiti, Nora Shipp +6

The Hercules ultra-faint dwarf galaxy (UFD) has long been hypothesized to be tidally disrupting, yet no conclusive evidence has been found for tidal disruption owing partly to diff…

astro-ph.GA2024

A Strontium-rich Ultra Metal-poor Star in the Atari Disk Component

Mohammad K. Mardini, Anna Frebel, Anirudh Chiti

We report on the discovery of the first ultra metal-poor (UMP) star 2MASS~J205001946613298 (J20506613; \mbox{[Fe/H] = }) selected from the Gaia BP/RP spectral catalog…

astro-ph.GA2024★ 22 cited

Enrichment by Extragalactic First Stars in the Large Magellanic Cloud

Anirudh Chiti, Mohammad Mardini, Guilherme Limberg +8

The Large Magellanic Cloud (LMC) is the Milky Way's most massive satellite galaxy, which only recently (~2 billion years ago) fell into our Galaxy. Since stellar atmospheres preser…

astro-ph.GA2023★ 3 cited

Metal-poor stars observed with the Magellan Telescope. IV. Neutron-capture element signatures in 27 main-sequence stars

Mohammad K. Mardini, Anna Frebel, Leyatt Betre +3

Based on high-resolution spectra obtained with Magellan/MIKE, we present a chemo-dynamical analysis for 27 near main-sequence turnoff metal-poor stars, including 20 stars analyzed…

astro-ph.GA2023★ 13 cited

The dark matter profile of the Milky Way inferred from its circular velocity curve

Xiaowei Ou, Anna-Christina Eilers, Lina Necib +1

In this paper, we construct the circular velocity curve of the Milky Way out to kpc, providing an updated model of the dark matter density profile. We derive precise para…

astro-ph.GA2022★ 31 cited

Timing the r-Process Enrichment of the Ultra-Faint Dwarf Galaxy Reticulum II

Joshua D. Simon, Thomas M. Brown, Burçin Mutlu-Pakdil +65

The ultra-faint dwarf galaxy Reticulum II (Ret II) exhibits a unique chemical evolution history, with 72 +10/-12% of its stars strongly enhanced in r-process elements. We present d…