activity
20122026
most citedThe GALAH+ Survey: Third Data Release

626 citations · 4.9k across the 107 of their papers we have counts for

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35 papers · 1 filter

astro-ph.GA2026

Detailed Abundance Determination of Metal-Poor Stars with X-Shooter II. - Chemically Disentangling the Halo, Disk and GSE

Benjamin D. C. Lowe, Luca Casagrande, Thomas Nordlander +2

We present a detailed chemical analysis of seven extremely metal-poor (EMP) star candidates observed with X-Shooter, combining them with 16 EMP candidates from Paper I. We measured…

astro-ph.GA2026★ 3 cited

The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios

M. McKenzie, D. Yong, A. I. Karakas +8

The complex star cluster M 22 (NGC 6656) provides a unique opportunity for studying slow neutron-capture (s-process) nucleosynthesis at low metallicity due to its two stellar group…

astro-ph.GA2026

The GALAH Survey: Neutron-Capture Elemental Abundances for 350,000 Gaia-RVS spectra and the Chemodynamics of Accreted Structures

Pradosh Barun Das, Daniel B. Zucker, Aldo Mura-Guzmán +15

We present a comprehensive data-driven spectroscopic analysis of 357,415 red giant stars using Gaia DR3 Radial Velocity Spectrometer (RVS) spectra (8460-8700 A; ),…

astro-ph.GA2025

Detailed Abundance Determination of Metal-Poor Stars with X-Shooter I. Unusual Chemistry in Halo Stars

Benjamin D. C. Lowe, Thomas Nordlander, Luca Casagrande +5

We present a detailed chemical analysis study of 16 candidate metal-poor stars, previously identified with 2dF + AAOmega, using X-Shooter spectra and the Korg 1D local thermodynami…

astro-ph.GA2025★ 3 cited

The Rise of the Milky Way Disk through EMP Stars

B. Lowe, T. Nordlander, L. Casagrande +6

We present a chemo-dynamical study conducted with 2dFAAOmega of Gaia DR3 non-variable candidate metal-poor stars that lie in the direction of the Galactic plane. Our…

astro-ph.GA2025★ 5 cited

The GALAH survey: Improving chemical abundances using star clusters

Janez Kos, Sven Buder, Kevin L. Beeson +18

Large spectroscopic surveys aim to consistently compute stellar parameters of very diverse stars while minimizing systematic errors. We explore the use of stellar clusters as bench…

astro-ph.GA2024★ 8 cited

The GALAH Survey: Stellar parameters and abundances for 800,000 Gaia RVS spectra using GALAH DR4 and The Cannon

Pradosh Barun Das, Daniel B. Zucker, Gayandhi M. De Silva +15

Analysing stellar parameters and abundances from nearly one million Gaia Data Release 3 (DR3) Radial Velocity Spectrometer (RVS) spectra poses challenges due to the limited spectra…

astro-ph.GA2024★ 11 cited

The GALAH Survey: Data Release 4

S. Buder, J. Kos, E. X. Wang +36

The stars of the Milky Way carry the chemical history of our Galaxy in their atmospheres as they journey through its vast expanse. Like barcodes, we can extract the chemical finger…

astro-ph.GA2022★ 13 cited

The impact of carbon and oxygen abundances on the metal-poor initial mass function

Piyush Sharda, Anish M. Amarsi, Kathryn Grasha +5

Star formation models predict that the metal-poor initial mass function (IMF) can be substantially different from that observed in the metal-rich Milky Way. This changeover occurs…

astro-ph.GA2022★ 81 cited

The Gaia-ESO survey: mapping the shape and evolution of the radial abundance gradients with open clusters

L. Magrini, C. Viscasillas Vazquez, L. Spina +27

The spatial distribution of elemental abundances and their time evolution are among the major constraints to disentangle the scenarios of formation and evolution of the Galaxy. We…

astro-ph.GA2022★ 9 cited

Spectroscopic follow-up of statistically selected extremely metal-poor star candidates from GALAH DR3

G. S. Da Costa, M. S. Bessell, Thomas Nordlander +5

The advent of large-scale stellar spectroscopic surveys naturally leads to the implementation of machine learning techniques to isolate, for example, small sub-samples of potential…

astro-ph.GA2022★ 8 cited

A method for identifying metal-poor stars with Gaia BP/RP spectra

Theodora Xylakis-Dornbusch, Norbert Christlieb, Karin Lind +1

Context. The study of the oldest and most metal-poor stars in our Galaxy promotes our understanding of the Galactic chemical evolution and the beginning of Galaxy and star formatio…

astro-ph.GA2022

The GALAH Survey: A New Sample of Extremely Metal-Poor Stars Using A Machine Learning Classification Algorithm

Arvind C. N. Hughes, Lee R. Spitler, Daniel B. Zucker +21

Extremely Metal-Poor (EMP) stars provide a valuable probe of early chemical enrichment in the Milky Way. Here we leverage a large sample of high-resolution stellar sp…

astro-ph.GA2021★ 93 cited

The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and eDR3

Sven Buder, Karin Lind, Melissa K. Ness +27

Since the advent of astrometry, it is possible to identify massive accreted systems within the Galaxy through their unique dynamical signatures. One such system, -Saus…

astro-ph.GA2021★ 38 cited

High resolution spectroscopic follow-up of the most metal-poor candidates from SkyMapper DR1.1

D. Yong, G. S. Da Costa, M. S. Bessell +13

We present chemical abundances for 21 elements (from Li to Eu) in 150 metal-poor Galactic stars spanning 4.1 [Fe/H] 2.1. The targets were selected from the SkyMapper…

astro-ph.GA2021★ 11 cited

The GALAH Survey: No chemical evidence of an extragalactic origin for the Nyx stream

Daniel B. Zucker, Jeffrey D. Simpson, Sarah L. Martell +20

The results from the ESA Gaia astrometric mission and deep photometric surveys have revolutionized our knowledge of the Milky Way. There are many ongoing efforts to search these da…

astro-ph.GA2020★ 38 cited

The GALAH Survey: Chemical Clocks

Michael R. Hayden, Sanjib Sharma, Joss Bland-Hawthorn +27

Previous studies have found that the elemental abundances of a star correlate directly with its age and metallicity. Using this knowledge, we derive ages for a sample of 250,000 st…

astro-ph.GA2020★ 50 cited

Milky Way Tomography with the SkyMapper Southern Survey. II. Photometric Re-calibration of SMSS DR2

Yang Huang, Haibo Yuan, Chengyuan Li +13

We apply the spectroscopy-based stellar-color regression (SCR) method to perform an accurate photometric re-calibration of the second data release from the SkyMapper Southern Surve…

astro-ph.GA2020★ 54 cited

Exploring the Galaxy's halo and very metal-weak thick disk with SkyMapper and Gaia DR2

G. Cordoni, G. S. Da Costa, D. Yong +16

In this work we combine spectroscopic information from the \textit{SkyMapper survey for Extremely Metal-Poor stars} and astrometry from Gaia DR2 to investigate the kinematics of a…

astro-ph.GA2020★ 27 cited

Combined APOGEE-GALAH stellar catalogues using the Cannon

Govind Nandakumar, Michael R. Hayden, Sanjib Sharma +21

APOGEE and GALAH are two high resolution multi-object spectroscopic surveys that provide fundamental stellar parameters and multiple elemental abundance estimates for about half a…

astro-ph.GA2020★ 21 cited

The GALAH Survey: Accreted stars also inhabit the Spite Plateau

Jeffrey D. Simpson, Sarah L. Martell, Sven Buder +22

The ESA Gaia astrometric mission has enabled the remarkable discovery that a large fraction of the stars near the Solar neighbourhood appear to be debris from a single in-falling s…

astro-ph.GA2020★ 117 cited

The GALAH survey: tracing the Galactic disk with Open Clusters

Lorenzo Spina, Yuan-Sen Ting, Gayandhi M. De Silva +28

Open clusters are unique tracers of the history of our own Galaxy's disk. According to our membership analysis based on \textit{Gaia} astrometry, out of the 226 potential clusters…

astro-ph.GA2020★ 626 cited

The GALAH+ Survey: Third Data Release

Sven Buder, Sanjib Sharma, Janez Kos +44

The ensemble of chemical element abundance measurements for stars, along with precision distances and orbit properties, provides high-dimensional data to study the evolution of the…

astro-ph.GA2020★ 45 cited

A Minimum Dilution Scenario for Supernovae and Consequences for Extremely Metal-Poor Stars

Mattis Magg, Thomas Nordlander, Simon C. O. Glover +6

To date no metal-free stars have been identified by direct observations. The most common method of constraining their properties is searching the spectra of the most metal-poor sta…