The GALAH survey: Data release 4
Artikel i vetenskaplig tidskrift, 2025

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 fingerprints of stars from high-resolution spectroscopy. The fourth data release (DR4) of the Galactic Archaeology with HERMES (GALAH) Survey, based on a decade of observations, provides the chemical abundances of up to 32 elements for 917 588 stars that also have exquisite astrometric data from the Gaia satellite. For the first time, these elements include life-essential nitrogen to complement carbon, and oxygen as well as more measurements of rare-earth elements critical to modern-life electronics, offering unparalleled insights into the chemical composition of the Milky Way. For this release, we use neural networks to simultaneously fit stellar parameters and abundances across the whole wavelength range, leveraging synthetic grids computed with Spectroscopy Made Easy. These grids account for atomic line formation in non-local thermodynamic equilibrium for 14 elements. In a two-iteration process, we first fit stellar labels to all 1 085 520 spectra, then co-add repeated observations and refine these labels using astrometric data from Gaia and 2MASS photometry, improving the accuracy and precision of stellar parameters and abundances. Our validation thoroughly assesses the reliability of spectroscopic measurements and highlights key caveats. GALAH DR4 represents yet another milestone in Galactic archaeology, combining detailed chemical compositions from multiple nucleosynthetic channels with kinematic information and age estimates. The resulting dataset, covering nearly a million stars, opens new avenues for understanding not only the chemical and dynamical history of the Milky Way but also the broader questions of the origin of elements and the evolution of planets, stars, and galaxies.

Surveys

methods: observational

methods: data analysis

stars: fundamental parameters

stars: abundances

the Galaxy

Författare

Sven Buder

Australian National University

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Janez Kos

Univerza V Ljubljani

Xi Ella Wang

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Australian National University

Madeleine Howell

Monash University

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Sarah Martell

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

University of New South Wales (UNSW)

Michael R. Hayden

The University of Sydney

University of New South Wales (UNSW)

University of Oklahoma

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Daniel B. Zucker

Macquarie University

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Thomas Nordlander

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Uppsala universitet

Australian National University

Benjamin Montet

University of New South Wales (UNSW)

Gregor Traven

Univerza V Ljubljani

Joss Bland-Hawthorn

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

The University of Sydney

Gayandhi M. De Silva

Macquarie University

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Kenneth Freeman

Australian National University

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Geraint Lewis

The University of Sydney

Karin Lind

Stockholms universitet

Sanjib Sharma

Space Telescope Science Institute (STScI)

Jeffrey D. Simpson

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

University of New South Wales (UNSW)

Dennis Stello

The University of Sydney

Aarhus Universitet

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

University of New South Wales (UNSW)

Tomaz Zwitter

Univerza V Ljubljani

Anish M. Amarsi

Uppsala universitet

Joseph Armstrong

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Kirsten Banks

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

University of New South Wales (UNSW)

Mark Beavis

University of Southern Queensland

Kevin-Luke Beeson

Univerza V Ljubljani

Boquan Chen

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Australian National University

Ioana Ciuca

Australian National University

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Gary S. Da Costa

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Australian National University

Richard de Grijs

Macquarie University

Int Space Sci Inst Beijing

Bailey Martin

Australian National University

David Moise Nataf

University of Iowa

Melissa Ness

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Australian National University

Adam D. Rains

Uppsala universitet

Tim Scarr

Australian National University

Zixian Purmortal Wang

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

University of Utah

The University of Sydney

Rob A. Wittenmyer

University of Southern Queensland

Yi Anne Xie

ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)

Australian National University

Publications Astronomical Society of Australia

1323-3580 (ISSN) 1448-6083 (eISSN)

Vol. 42 e051

Ämneskategorier (SSIF 2025)

Astronomi, astrofysik och kosmologi

DOI

10.1017/pasa.2025.26

Mer information

Senast uppdaterat

2025-06-13