Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc

dc.contributor.authorAnders, Friedrich
dc.contributor.authorGispert, P.
dc.contributor.authorRatcliffe, Bridget
dc.contributor.authorChiappini, C.
dc.contributor.authorMinchev, I.
dc.contributor.authorNepal, Samir
dc.contributor.authorQueiroz, A. B. A.
dc.contributor.authorAmarante, João Antônio Silveira do
dc.contributor.authorAntoja Castelltort, M. Teresa
dc.contributor.authorCasali, Giada
dc.contributor.authorCasamiquela, L.
dc.contributor.authorKhalatyan, A.
dc.contributor.authorMiglio, A.
dc.contributor.authorPerottoni, Helio
dc.contributor.authorSchultheis, M.
dc.date.accessioned2025-07-22T11:12:59Z
dc.date.available2025-07-22T11:12:59Z
dc.date.issued2023-10
dc.date.updated2025-07-22T11:12:59Z
dc.description.abstractOver the last few years, many studies have found an empirical relationship between the abundance of a star and its age. Here we estimate spectroscopic stellar ages for 178 825 red-giant stars observed by the APOGEE survey with a median statistical uncertainty of 17%. To this end, we use the supervised machine learning technique XGBoost, trained on a high-quality dataset of 3060 redgiant and red-clump stars with asteroseismic ages observed by both APOGEE and Kepler. After verifying the obtained age estimates with independent catalogues, we investigate some of the classical chemical, positional, and kinematic relationships of the stars as a function of their age. We find a very clear imprint of the outer-disc flare in the age maps and confirm the recently found split in the local age-metallicity relation. We present new and precise measurements of the Galactic radial metallicity gradient in small age bins between 0.5 and 12 Gyr, confirming a steeper metallicity gradient for ∼2−5 Gyr old populations and a subsequent flattening for older populations mostly produced by radial migration. In addition, we analyse the dispersion about the abundance gradient as a function of age. We find a clear power-law trend (with an exponent β ≈ 0.15) for this relation, indicating a relatively smooth radial migration history in the Galactic disc over the past 7−9 Gyr. Departures from this power law may possibly be related to the Gaia Enceladus merger and passages of the Sagittarius dSph galaxy. Finally, we confirm previous measurements showing a steepening in the agevelocity dispersion relation at around ∼9 Gyr, but now extending it over a large extent of the Galactic disc (5 kpc < RGal < 13 kpc). To establish whether this steepening is the imprint of a Galactic merger event, however, detailed forward modelling work of our data is necessary. Our catalogue of precise stellar ages and the source code to create it are publicly available.
dc.format.extent21 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec746882
dc.identifier.issn0004-6361
dc.identifier.urihttps://hdl.handle.net/2445/222474
dc.language.isoeng
dc.publisherEDP Sciences
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1051/0004-6361/202346666
dc.relation.ispartofAstronomy & Astrophysics, 2023, vol. 678
dc.relation.urihttps://doi.org/10.1051/0004-6361/202346666
dc.rights(c) The European Southern Observatory (ESO), 2023
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationEvolució de les galàxies
dc.subject.classificationClassificació dels estels
dc.subject.classificationEvolució estel·lar
dc.subject.otherGalaxies evolution
dc.subject.otherStar Classification
dc.subject.otherStellar evolution
dc.titleSpectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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