Podrobno

The GALAH survey : data release 4
ID Buder, Sven (Avtor), ID Kos, Janez (Avtor), ID Zwitter, Tomaž (Avtor), ID Beeson, Kevin Luke (Avtor), ID Vogrinčič, Rok (Avtor)

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.pdfPDF - Predstavitvena datoteka, prenos (6,79 MB)
MD5: F2C6935F19EED9B3010AD32ECD1F4B27

Izvleček
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.

Jezik:Angleški jezik
Ključne besede:surveys, Galaxy, fundamental parameters
Vrsta gradiva:Članek v reviji
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:FMF - Fakulteta za matematiko in fiziko
Status publikacije:Objavljeno
Različica publikacije:Objavljena publikacija
Datum objave:01.05.2025
Leto izida:2025
Št. strani:42 str.
Številčenje:Vol. 42, art. id. ǂe051
PID:20.500.12556/RUL-169937 Povezava se odpre v novem oknu
UDK:524.6
ISSN pri članku:1448-6083
DOI:10.1017/pasa.2025.26 Povezava se odpre v novem oknu
COBISS.SI-ID:240010499 Povezava se odpre v novem oknu
Datum objave v RUL:19.06.2025
Število ogledov:281
Število prenosov:45
Metapodatki:XML DC-XML DC-RDF
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Gradivo je del revije

Naslov:Publications of the Astronomical Society of Australia
Založnik:CSIRO Publishing
ISSN:1448-6083
COBISS.SI-ID:521631513 Povezava se odpre v novem oknu

Licence

Licenca:CC BY 4.0, Creative Commons Priznanje avtorstva 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by/4.0/deed.sl
Opis:To je standardna licenca Creative Commons, ki daje uporabnikom največ možnosti za nadaljnjo uporabo dela, pri čemer morajo navesti avtorja.

Sekundarni jezik

Jezik:Slovenski jezik
Ključne besede:pregledi, Galaksija, osnovni parametri

Projekti

Financer:ARIS - Javna agencija za znanstvenoraziskovalno in inovacijsko dejavnost Republike Slovenije
Številka projekta:P1-0188-2022
Naslov:Astrofizika in fizika atmosfere

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