The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission
文献类型:期刊论文
作者 | Gent, Matthew Raymond26; Bergemann, Maria13,26; Serenelli, Aldo1,14,26; Casagrande, Luca4; Gerber, Jeffrey M.26; Heiter, Ulrike12; Kovalev, Mikhail10,26; Morel, Thierry2; Nardetto, Nicolas3; Adibekyan, Vardan18,20 |
刊名 | ASTRONOMY & ASTROPHYSICS |
出版日期 | 2022-02-11 |
卷号 | 658 |
ISSN号 | 0004-6361 |
关键词 | surveys stars: fundamental parameters stars: solar-type stars: abundances stars: atmospheres |
DOI | 10.1051/0004-6361/202140863 |
产权排序 | 第23完成单位 |
文献子类 | Article |
英文摘要 | We introduce the SAPP (Stellar Abundances and atmospheric Parameters Pipeline), the prototype of the code that will be used to determine parameters of stars observed within the core program of the PLATO space mission. The pipeline is based on the Bayesian inference and provides effective temperature, surface gravity, metallicity, chemical abundances, and luminosity. The code in its more general version has a much wider range of potential applications. It can also provide masses, ages, and radii of stars and can be used with stellar types not targeted by the PLATO core program, such as red giants. We validate the code on a set of 27 benchmark stars that includes 19 FGK-type dwarfs, 6 GK-type subgiants, and 2 red giants. Our results suggest that combining various observables is the optimal approach, as this allows the degeneracies between different parameters to be broken and yields more accurate values of stellar parameters and more realistic uncertainties. For the PLATO core sample, we obtain a typical uncertainty of 27 (syst.) +/- 37 (stat.) K for T-eff, 0.00 +/- 0.01 dex for log g, 0.02 +/- 0.02 dex for metallicity [Fe/H], -0.01 +/- 0.03 R-circle dot for radii, -0.01 +/- 0.05 M-circle dot for stellar masses, and -0.14 +/- 0.63 Gyr for ages. We also show that the best results are obtained by combining the nu(max) scaling relation with stellar spectra. This resolves the notorious problem of degeneracies, which is particularly important for F-type stars. |
学科主题 | 天文学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE |
WOS关键词 | BRIGHTNESS-COLOR RELATIONS ; LTE LINE FORMATION ; ACCURATE FUNDAMENTAL PARAMETERS ; SAMPLING MODEL ATMOSPHERES ; SOLAR-LIKE OSCILLATIONS ; INFRARED FLUX METHOD ; MAIN-SEQUENCE ; CHEMICAL ABUNDANCES ; IONIZATION BALANCE ; ANGULAR DIAMETERS |
资助项目 | Max Planck SocietyMax Planck SocietyFoundation CELLEX ; CNES, the Centre National d'Etudes Spatiales ; Collaborative Research centre, Heidelberg University ; Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)German Research Foundation (DFG) ; MICINNSpanish GovernmentEuropean Commission[PID2019-108709GB-I00] ; BelspoBelgian Federal Science Policy Office ; Swedish National Space Agency (SNSA/Rymdstyrelsen) ; Janos Bolyai Research Scholarship of the Hungarian Academy of SciencesHungarian Academy of Sciences ; New National Excellence Program of the Ministry for Innovation and Technology[UNKP-20-5] ; FCT -Fundacao para a Ciencia e Tecnologia (FCT)[UID/FIS/04434/2019] ; FCT -Fundacao para a Ciencia e Tecnologia (FCT)[UIDB/04434/2020] ; FCT -Fundacao para a Ciencia e Tecnologia (FCT)[UIDP/04434/2020] ; FCTPortuguese Foundation for Science and TechnologyEuropean Commission[IF/00650/2015/CP1273/CT0001] ; MIURMinistry of Education, Universities and Research (MIUR) ; ARC Future FellowshipAustralian Research Council[FT160100402] ; European Research Council (ERC) under the European UnionEuropean Research Council (ERC)[949173] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | EDP SCIENCES S A |
WOS记录号 | WOS:000754052500001 |
资助机构 | Max Planck SocietyMax Planck SocietyFoundation CELLEX ; CNES, the Centre National d'Etudes Spatiales ; Collaborative Research centre, Heidelberg University ; Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)German Research Foundation (DFG) ; MICINNSpanish GovernmentEuropean Commission[PID2019-108709GB-I00] ; BelspoBelgian Federal Science Policy Office ; Swedish National Space Agency (SNSA/Rymdstyrelsen) ; Janos Bolyai Research Scholarship of the Hungarian Academy of SciencesHungarian Academy of Sciences ; New National Excellence Program of the Ministry for Innovation and Technology[UNKP-20-5] ; FCT -Fundacao para a Ciencia e Tecnologia (FCT)[UID/FIS/04434/2019, UIDB/04434/2020, UIDP/04434/2020] ; FCTPortuguese Foundation for Science and TechnologyEuropean Commission[IF/00650/2015/CP1273/CT0001] ; MIURMinistry of Education, Universities and Research (MIUR) ; ARC Future FellowshipAustralian Research Council[FT160100402] ; European Research Council (ERC) under the European UnionEuropean Research Council (ERC)[949173] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/24916] |
专题 | 云南天文台_大样本恒星演化研究组 |
通讯作者 | Gent, Matthew Raymond |
作者单位 | 1.Institut d’Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, 08034 Barcelona, Spain; 2.Space Sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège, Quartier Agora, Allée du 6 Août 19c, Bât. B5C, 4000 Liège, Belgium; 3.Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Lagrange, CS 34229, Nice, France; 4.Research School of Astronomy & Astrophysics, Mount Stromlo Observatory, Australian National University, ACT 2611, Australia; 5.Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, CP 226, Boulevard du Triomphe, 1050 Brussels, Belgium; 6.ELTE Eötvös Loránd University, Gothard Astrophysical Observatory, Szent Imre H. St. 112, 9700 Szombathely, Hungary; 7.LESIA, Observatoire de Paris, Bât. 14 – Soleil-Planètes, 5 Place Jules Janssen, 92195 Meudon, France 8.Space Science Institute, 4765 Walnut Street, Boulder, CO 80301, USA; 9.Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120/1520, 8000 Aarhus, Denmark; 10.Yunnan Observatories, Chinese Academy of Sciences, PO Box 110 Kunming 650216, PR China; |
推荐引用方式 GB/T 7714 | Gent, Matthew Raymond,Bergemann, Maria,Serenelli, Aldo,et al. The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission[J]. ASTRONOMY & ASTROPHYSICS,2022,658. |
APA | Gent, Matthew Raymond.,Bergemann, Maria.,Serenelli, Aldo.,Casagrande, Luca.,Gerber, Jeffrey M..,...&Tsantaki, Maria.(2022).The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission.ASTRONOMY & ASTROPHYSICS,658. |
MLA | Gent, Matthew Raymond,et al."The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission".ASTRONOMY & ASTROPHYSICS 658(2022). |
入库方式: OAI收割
来源:云南天文台
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