StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars
This article has an erratum: [https://doi.org/10.1051/0004-6361/202245399e]
| Autores: | , , , , , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/348941 |
| Acceso en línea: | http://hdl.handle.net/10261/348941 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxy: disk Stars: abundances Solar neighborhood Galaxy: general Methods: statistical Galaxy: stellar content |
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| dc.title.none.fl_str_mv |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| title |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| spellingShingle |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars Queiroz, Anna Bárbara de Andrade Galaxy: disk Stars: abundances Solar neighborhood Galaxy: general Methods: statistical Galaxy: stellar content |
| title_short |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| title_full |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| title_fullStr |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| title_full_unstemmed |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| title_sort |
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars |
| dc.creator.none.fl_str_mv |
Queiroz, Anna Bárbara de Andrade Anders, Friedrich Chiappini, Cristina Khalatyan, A. Santiago, Basílio Xavier Nepal, Samir Steinmetz, Matthias Gallart, C. Valentini, Martina Dal Ponte, M. Barbuy, Beatriz Pérez-Villegas, Angeles Masseron, Thomas Fernández-Trincado, J. G. Khoperskov, Sergey Minchev, Ivan Fernández Alvar, Emma Lane, Richard R. Nitschelm, Christian |
| author |
Queiroz, Anna Bárbara de Andrade |
| author_facet |
Queiroz, Anna Bárbara de Andrade Anders, Friedrich Chiappini, Cristina Khalatyan, A. Santiago, Basílio Xavier Nepal, Samir Steinmetz, Matthias Gallart, C. Valentini, Martina Dal Ponte, M. Barbuy, Beatriz Pérez-Villegas, Angeles Masseron, Thomas Fernández-Trincado, J. G. Khoperskov, Sergey Minchev, Ivan Fernández Alvar, Emma Lane, Richard R. Nitschelm, Christian |
| author_role |
author |
| author2 |
Anders, Friedrich Chiappini, Cristina Khalatyan, A. Santiago, Basílio Xavier Nepal, Samir Steinmetz, Matthias Gallart, C. Valentini, Martina Dal Ponte, M. Barbuy, Beatriz Pérez-Villegas, Angeles Masseron, Thomas Fernández-Trincado, J. G. Khoperskov, Sergey Minchev, Ivan Fernández Alvar, Emma Lane, Richard R. Nitschelm, Christian |
| author2_role |
author author author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
European Space Agency Ministerio de Ciencia e Innovación (España) Ministerio de Ciencia, Innovación y Universidades (España) Agencia Estatal de Investigación (España) European Commission Gobierno de Canarias Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Galaxy: disk Stars: abundances Solar neighborhood Galaxy: general Methods: statistical Galaxy: stellar content |
| topic |
Galaxy: disk Stars: abundances Solar neighborhood Galaxy: general Methods: statistical Galaxy: stellar content |
| description |
This article has an erratum: [https://doi.org/10.1051/0004-6361/202245399e] |
| publishDate |
2023 |
| dc.date.none.fl_str_mv |
2023 2024 2024 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
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http://hdl.handle.net/10261/348941 |
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http://hdl.handle.net/10261/348941 |
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Inglés |
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Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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EDP Sciences |
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StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich starsQueiroz, Anna Bárbara de AndradeAnders, FriedrichChiappini, CristinaKhalatyan, A.Santiago, Basílio XavierNepal, SamirSteinmetz, MatthiasGallart, C.Valentini, MartinaDal Ponte, M.Barbuy, BeatrizPérez-Villegas, AngelesMasseron, ThomasFernández-Trincado, J. G.Khoperskov, SergeyMinchev, IvanFernández Alvar, EmmaLane, Richard R.Nitschelm, ChristianGalaxy: diskStars: abundancesSolar neighborhoodGalaxy: generalMethods: statisticalGalaxy: stellar contentThis article has an erratum: [https://doi.org/10.1051/0004-6361/202245399e]The Gaia mission has provided an invaluable wealth of astrometric data for more than a billion stars in our Galaxy. The synergy between Gaia astrometry, photometry, and spectroscopic surveys gives us comprehensive information about the Milky Way. Using the Bayesian isochrone-fitting code StarHorse, we derive distances and extinctions for more than 10 million unique stars listed in both Gaia Data Release 3 and public spectroscopic surveys: 557 559 in GALAH+ DR3, 4 531 028 in LAMOST DR7 LRS, 347 535 in LAMOST DR7 MRS, 562 424 in APOGEE DR17, 471 490 in RAVE DR6, 249 991 in SDSS DR12 (optical spectra from BOSS and SEGUE), 67 562 in the Gaia-ESO DR5 survey, and 4 211 087 in the Gaia RVS part of the Gaia DR3 release. StarHorse can increase the precision of distance and extinction measurements where Gaia parallaxes alone would be uncertain. We used StarHorse for the first time to derive stellar ages for main-sequence turnoff and subgiant branch stars, around 2.5 million stars, with age uncertainties typically around 30%; the uncertainties drop to 15% for subgiant-branch-only stars, depending on the resolution of the survey. With the derived ages in hand, we investigated the chemical-age relations. In particular, the α and neutron-capture element ratios versus age in the solar neighbourhood show trends similar to previous works, validating our ages. We used the chemical abundances from local subgiant samples of GALAH DR3, APOGEE DR17, and LAMOST MRS DR7 to map groups with similar chemical compositions and StarHorse ages, using the dimensionality reduction technique t-SNE and the clustering algorithm HDBSCAN. We identify three distinct groups in all three samples, confirmed by their kinematic properties: the genuine chemical thick disk, the thin disk, and a considerable number of young alpha-rich stars (427) that are also a part of the delivered catalogues. We confirm that the genuine thick disk’s kinematics and age properties are radically different from those of the thin disk and compatible with high-redshift (z ≈ 2) star-forming disks with high dispersion velocities. We also find a few extra chemical populations in GALAH DR3 thanks to the availability of neutron-capture element information.This work was partially supported by the Spanish Ministry of Science, Innovation and University (MICIU/FEDER, UE) through grant RTI2018-095076-B-C21, and the Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia ‘María de Maeztu’) through grant CEX2019-000918-M. F.A. acknowledges financial support from MICINN (Spain) through the Juan de la Cierva-Incorporcion programme under contract IJC2019-04862-I. A.P.-V. acknowledges the DGAPA-PAPIIT grant IA103122. T.M. acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) through the Spanish State Research Agency, under the Severo Ochoa Program 2020-2023 (CEX2019-000920-S) as well as support from the ACIISI, Consejería de Economía, Conocimiento y Empleo del Gobierno de Canarias and the European Regional Development Fund (ERDF) under grant with reference PROID2021010128. C.G. and E.F.A. acknowledge support from the Agencia Estatal de Investigación del Ministerio de Ciencia e Innovación (AEI-MCINN) under grant “At the forefront of Galactic Archaeology: evolution of the luminous and dark matter components of the Milky Way and Local Group dwarf galaxies in the Gaia era” with reference PID2020-118778GBI00/10.13039/501100011033. C.G. also acknowledges support from the Severo Ochoa program through CEX2019-000920-S. EFA also acknowleges support from the ‘María Zambrano’ fellowship from the Universidad de La Laguna.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2019-000918-M).With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2019-000920-S).Peer reviewedEDP SciencesEuropean Space AgencyMinisterio de Ciencia e Innovación (España)Ministerio de Ciencia, Innovación y Universidades (España)Agencia Estatal de Investigación (España)European CommissionGobierno de CanariasConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242023info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/348941reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/RTI2018-095076-B-C21info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2019-000918-Minfo:eu-repo/grantAgreement/AEI//JC2019-04862-Iinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2019-000920-Sinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-118778GB-I00The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1051/0004-6361/202245399https://doi.org/10.1051/0004-6361/202245399Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3489412026-05-22T06:33:51Z |
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