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The GALAH survey : stellar parameters and abundances for 800 000 Gaia RVS spectra using GALAH DR4 and The Cannon
ID
Das, Pradosh Barun
(
Avtor
),
ID
Zucker, Daniel B.
(
Avtor
),
ID
De Silva, Gayandhi M.
(
Avtor
),
ID
Borsato, Nicholas W.
(
Avtor
),
ID
Mura-Guzman, Aldo
(
Avtor
),
ID
Buder, Sven
(
Avtor
),
ID
Kos, Janez
(
Avtor
)
PDF - Predstavitvena datoteka,
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MD5: 57263B65CD8C07BDC9A42D779986F6AB
URL - Izvorni URL, za dostop obiščite
https://academic.oup.com/mnras/article-pdf/538/2/605/61706695/staf169.pdf
Galerija slik
Izvleček
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 spectral coverage (restricted to the infrared Ca II triplet) and variable signal-to-noise ratios of the data. To address this, we use The Cannon, a data-driven method, to transfer stellar parameters and abundances from the GALAH (GALactic Archaeology with HERMES) DR4 (R ∼ 28 000) catalogue to the lower resolution Gaia DR3 RVS spectra (R ∼ 11 500). Our model, trained on 14 484 common targets, predicts parameters such as Teff , log g, and [Fe/H], along with several other elements across approximately 800 000 Gaia RVS spectra. We utilize stars from open and globular clusters present in the Gaia RVS catalogue to validate our predicted mean [Fe/H] with high precision (∼ 0.02−0.10 dex). Additionally, we recover the bimodal distribution of [Ti/Fe] versus [Fe/H], reflecting the high and low α-components of Milky Way disc stars, demonstrating The Cannon’s capability for accurate stellar abundance determination from medium-resolution Gaia RVS spectra. The methodologies and resultant catalogue presented in this work highlight the remarkable potential of the RVS data set, which by the end of the Gaia mission will comprise spectra of over 200 million stars.
Jezik:
Angleški jezik
Ključne besede:
astrophysics of galaxies
,
spectroscopic survey
Vrsta gradiva:
Članek v reviji
Tipologija:
1.01 - Izvirni znanstveni članek
Organizacija:
FMF - Fakulteta za matematiko in fiziko
Status publikacije:
Objavljeno
Datum objave:
01.04.2025
Leto izida:
2025
Št. strani:
16 str.
Številčenje:
Vol. 538, issue 2
PID:
20.500.12556/RUL-168911
UDK:
524.8
ISSN pri članku:
1365-2966
DOI:
10.1093/mnras/staf169
COBISS.SI-ID:
234816003
Datum objave v RUL:
06.05.2025
Število ogledov:
349
Število prenosov:
82
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Objavi na:
Gradivo je del revije
Naslov:
Monthly notices of the Royal Astronomical Society
Skrajšan naslov:
Mon. not. R. Astron. Soc.
Založnik:
Blackwell Science
ISSN:
1365-2966
COBISS.SI-ID:
1870180
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