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20182026
most citedThe Atari Disk, a Metal-Poor Stellar Population in the Disk System of the Milky Way

51 citations · 494 across the 33 of their papers we have counts for

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23 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★ 1 cited

Galactic Archaeology with the Subaru `Ōnohi`ula Prime Focus Spectrograph Strategic Program

Masashi Chiba, Rosemary F. G. Wyse, Evan N. Kirby +48

The recently commissioned Subaru `Ōnohi`ula Prime Focus Spectrograph (PFS) will obtain spectra from nearly 2,400 fibers that cover 1.24 square degrees. The 360 night Subaru Strateg…

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

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.GA2024★ 3 cited

Cosmological insights into the early accretion of r-process-enhanced stars II. Dynamical identification of lost members of Reticulum II

P. Berczik, M. Ishchenko, O. Sobodar +1

Aims. We identify the possible dynamical connection between individual r-process-enhanced stars and the ultra-faint dwarf galaxy Reticulum II based on the current phase-space infor…

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

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

Unraveling the Origins and Development of the Galactic Disk through Metal-Poor Stars

Maria Rah, Manolya Yatman, Ali Taani +2

The Milky Way is a spiral galaxy comprising three main components: the Bulge, the Disk, and the Halo. Of particular interest is the Galactic disk, which holds a significant portion…

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★ 19 cited

Candidate Members of the VMP/EMP Disk System of the Galaxy from the SkyMapper and SAGES Surveys

Jihye Hong, Timothy C. Beers, Young Sun Lee +15

Photometric stellar surveys now cover a large fraction of the sky, probe to fainter magnitudes than large-scale spectroscopic surveys, and are relatively free from the target-selec…

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.GA2022★ 31 cited

The chemical abundance pattern of the extremely metal-poor thin disk star 2MASS J1808-5104 and its origins

Mohammad K. Mardini, Anna Frebel, Rana Ezzeddine +6

We present a high-resolution (), high signal-to-noise () Magellan/MIKE spectrum of the bright extremely metal-poor star 2MASS~J18085104. We find [Fe/H] = $…

astro-ph.GA2022★ 22 cited

Possibilities and Limitations of Kinematically Identifying Stars from Accreted Ultra-Faint Dwarf Galaxies

Kaley Brauer, Hillary Diane Andales, Alexander P. Ji +4

The Milky Way has accreted many ultra-faint dwarf galaxies (UFDs), and stars from these galaxies can be found throughout our Galaxy today. Studying these stars provides insight int…

astro-ph.GA2022★ 51 cited

The Atari Disk, a Metal-Poor Stellar Population in the Disk System of the Milky Way

Mohammad K. Mardini, Anna Frebel, Anirudh Chiti +3

We have developed a chemo-dynamical approach to assign 36,010 metal-poor SkyMapper stars to various Galactic stellar populations. Using two independent techniques (velocity and act…

astro-ph.GA2022★ 34 cited

Detailed chemical abundances of stars in the outskirts of the Tucana II ultra-faint dwarf galaxy

Anirudh Chiti, Anna Frebel, Alexander P. Ji +6

We present chemical abundances and velocities of five stars between 0.3 kpc to 1.1 kpc from the center of the Tucana II ultra-faint dwarf galaxy (UFD) from high-resolution Magellan…

astro-ph.GA2021★ 43 cited

Stellar Metallicities from SkyMapper Photometry II: Precise photometric metallicities of 280,000 giant stars with [Fe/H] in the Milky Way

Anirudh Chiti, Anna Frebel, Mohammad K. Mardini +3

The Milky Way's metal-poor stars are nearby ancient objects that are used to study early chemical evolution and the assembly and structure of the Milky Way. Here we present reliabl…

astro-ph.GA2021★ 27 cited

The Metal-Poor Metallicity Distribution of the Ancient Milky Way

Anirudh Chiti, Mohammad K. Mardini, Anna Frebel +1

We present a low metallicity map of the Milky Way consisting of 111,000 giants with [Fe/H] 0.75, based on public photometry from the second data r…

astro-ph.GA2021★ 15 cited

Metal-poor Stars Observed with the Automated Planet Finder Telescope. III. CEMP-no Stars are the Descendant of Population III Stars

Nour Aldein Almusleh, Ali Taani, Sergen Özdemir +4

In this study, we report a probabilistic insight into the stellar mass and supernovae (SNe) explosion energy of the possible progenitors of five CEMP-no stars. This was done by a d…

astro-ph.GA2020★ 36 cited

Cosmological Insights into the Early Accretion of \textit{r}-Process-Enhanced stars. I. A Comprehensive Chemo-dynamical Analysis of LAMOST J1109+0754

Mohammad K. Mardini, Vinicius M. Placco, Yohai Meiron +10

This study presents a comprehensive chemo-dynamical analysis of LAMOST J1109+0754, a bright (V = 12.8), extremely metal-poor (\abund{Fe}{H} = ) star, with a strong \textit{r…

astro-ph.GA2019★ 34 cited

Metal-poor Stars Observed with the Automated Planet Finder Telescope. II. Chemodynamical Analysis of Six Low-Metallicity Stars in the Halo System of the Milky Way

Mohammad K. Mardini, Vinicius M. Placco, Ali Taani +2

In this work, we study the chemical compositions and kinematic properties of six metal-poor stars with [Fe/H] in the Galactic halo. From high-resolution (R ~110,000)…

astro-ph.GA2019★ 38 cited

Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST

Mohammad K. Mardini, Haining Li, Vinicius M. Placco +6

We report on the discovery of five carbon-enhanced metal-poor (CEMP) stars in the metallicity range of [Fe/H] . These stars were selected from the LAMOST DR3 low-res…