Gaia Early Data Release 3. The Galactic anticentre

Antoja, T. and McMillan, P. J. and Kordopatis, G. and Ramos, P. and Helmi, A. and Balbinot, E. and Cantat-Gaudin, T. and Chemin, L. and Figueras, F. and Jordi, C. and Khanna, S. and Romero-Gómez, M. and Seabroke, G. M. and Brown, A. G. A. and Vallenari, A. and Prusti, T. and de Bruijne, J. H. J. and Babusiaux, C. and Biermann, M. and Creevey, O. L. and Evans, D. W. and Eyer, L. and Hutton, A. and Jansen, F. and Klioner, S. A. and Lammers, U. and Lindegren, L. and Luri, X. and Mignard, F. and Panem, C. and Pourbaix, D. and Randich, S. and Sartoretti, P. and Soubiran, C. and Walton, N. A. and Arenou, F. and Bailer-Jones, C. A. L. and Bastian, U. and Cropper, M. and Drimmel, R. and Katz, D. and Lattanzi, M. G. and van Leeuwen, F. and Bakker, J. and Castañeda, J. and De Angeli, F. and Ducourant, C. and Fabricius, C. and Fouesneau, M. and Frémat, Y. and Guerra, R. and Guerrier, A. and Guiraud, J. and Jean-Antoine Piccolo, A. and Masana, E. and Messineo, R. and Mowlavi, N. and Nicolas, C. and Nienartowicz, K. and Pailler, F. and Panuzzo, P. and Riclet, F. and Roux, W. and Sordo, R. and Tanga, P. and Thévenin, F. and Gracia-Abril, G. and Portell, J. and Teyssier, D. and Altmann, M. and Andrae, R. and Bellas-Velidis, I. and Benson, K. and Berthier, J. and Blomme, R. and Brugaletta, E. and Burgess, P. W. and Busso, G. and Carry, B. and Cellino, A. and Cheek, N. and Clementini, G. and Damerdji, Y. and Davidson, M. and Delchambre, L. and Dell’Oro, A. and Fernández-Hernández, J. and Galluccio, L. and García-Lario, P. and Garcia-Reinaldos, M. and González-Núñez, J. and Gosset, E. and Haigron, R. and Halbwachs, J.-L. and Hambly, N. C. and Harrison, D. 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J. and Cornez, T. and Cowell, S. and Crifo, F. and Crosta, M. and Crowley, C. and Dafonte, C. and Dapergolas, A. and David, M. and David, P. and de Laverny, P. and De Luise, F. and De March, R. and De Ridder, J. and de Souza, R. and de Teodoro, P. and de Torres, A. and del Peloso, E. F. and del Pozo, E. and Delgado, A. and Delgado, H. E. and Delisle, J.-B. and Di Matteo, P. and Diakite, S. and Diener, C. and Distefano, E. and Dolding, C. and Eappachen, D. and Enke, H. and Esquej, P. and Fabre, C. and Fabrizio, M. and Faigler, S. and Fedorets, G. and Fernique, P. and Fienga, A. and Fouron, C. and Fragkoudi, F. and Fraile, E. and Franke, F. and Gai, M. and Garabato, D. and Garcia-Gutierrez, A. and García-Torres, M. and Garofalo, A. and Gavras, P. and Gerlach, E. and Geyer, R. and Giacobbe, P. and Gilmore, G. and Girona, S. and Giuffrida, G. and Gomez, A. and Gonzalez-Santamaria, I. and González-Vidal, J. J. and Granvik, M. and Gutiérrez-Sánchez, R. and Guy, L. P. and Hauser, M. and Haywood, M. and Hidalgo, S. L. and Hilger, T. and Hładczuk, N. and Hobbs, D. and Holland, G. and Huckle, H. E. and Jasniewicz, G. and Jonker, P. G. and Juaristi Campillo, J. and Julbe, F. and Karbevska, L. and Kervella, P. and Kochoska, A. and Kontizas, M. and Korn, A. J. and Kostrzewa-Rutkowska, Z. and Kruszyńska, K. and Lambert, S. and Lanza, A. F. and Lasne, Y. and Le Campion, J.-F. and Le Fustec, Y. and Lebreton, Y. and Lebzelter, T. and Leccia, S. and Leclerc, N. and Lecoeur-Taibi, I. and Liao, S. and Licata, E. and Lindstrøm, H. E. P. and Lister, T. A. and Livanou, E. and Lobel, A. and Madrero Pardo, P. and Managau, S. and Mann, R. G. and Marchant, J. M. and Marconi, M. and Marcos Santos, M. M. S. and Marinoni, S. and Marocco, F. and Marshall, D. J. and Martin Polo, L. and Martín-Fleitas, J. M. and Masip, A. and Massari, D. and Mastrobuono-Battisti, A. and Mazeh, T. and Messina, S. and Michalik, D. and Millar, N. 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A. and Sadowski, G. and Sagristà Sellés, A. and Sahlmann, J. and Salgado, J. and Salguero, E. and Samaras, N. and Sanchez Gimenez, V. and Sanna, N. and Santoveña, R. and Sarasso, M. and Schultheis, M. and Sciacca, E. and Segol, M. and Segovia, J. C. and Ségransan, D. and Semeux, D. and Siddiqui, H. I. and Siebert, A. and Siltala, L. and Slezak, E. and Smart, R. L. and Solano, E. and Solitro, F. and Souami, D. and Souchay, J. and Spagna, A. and Spoto, F. and Steele, I. A. and Steidelmüller, H. and Stephenson, C. A. and Süveges, M. and Szabados, L. and Szegedi-Elek, E. and Taris, F. and Tauran, G. and Taylor, M. B. and Teixeira, R. and Thuillot, W. and Tonello, N. and Torra, F. and Torra, J. and Turon, C. and Unger, N. and Vaillant, M. and van Dillen, E. and Vanel, O. and Vecchiato, A. and Viala, Y. and Vicente, D. and Voutsinas, S. and Weiler, M. and Wevers, T. and Wyrzykowski, Ł. and Yoldas, A. and Yvard, P. and Zhao, H. and Zorec, J. and Zucker, S. and Zurbach, C. and Zwitter, T. (2021) Gaia Early Data Release 3. The Galactic anticentre. Astronomy and Astrophysics, 649 . Art. No. A8. ISSN 0004-6361. doi:10.1051/0004-6361/202039714. https://resolver.caltech.edu/CaltechAUTHORS:20210510-070722783

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Abstract

Aims. We aim to demonstrate the scientific potential of the Gaia Early Data Release 3 (EDR3) for the study of different aspects of the Milky Way structure and evolution and we provide, at the same time, a description of several practical aspects of the data and examples of their usage. Methods. We used astrometric positions, proper motions, parallaxes, and photometry from EDR3 to select different populations and components and to calculate the distances and velocities in the direction of the anticentre. In this direction, the Gaia astrometric data alone enable the calculation of the vertical and azimuthal velocities; also, the extinction is relatively low compared to other directions in the Galactic plane. We then explore the disturbances of the current disc, the spatial and kinematical distributions of early accreted versus in situ stars, the structures in the outer parts of the disc, and the orbits of open clusters Berkeley 29 and Saurer 1. Results. With the improved astrometry and photometry of EDR3, we find that: (i) the dynamics of the Galactic disc are very complex with oscillations in the median rotation and vertical velocities as a function of radius, vertical asymmetries, and new correlations, including a bimodality with disc stars with large angular momentum moving vertically upwards from below the plane, and disc stars with slightly lower angular momentum moving preferentially downwards; (ii) we resolve the kinematic substructure (diagonal ridges) in the outer parts of the disc for the first time; (iii) the red sequence that has been associated with the proto-Galactic disc that was present at the time of the merger with Gaia-Enceladus-Sausage is currently radially concentrated up to around 14 kpc, while the blue sequence that has been associated with debris of the satellite extends beyond that; (iv) there are density structures in the outer disc, both above and below the plane, most probably related to Monoceros, the Anticentre Stream, and TriAnd, for which the Gaia data allow an exhaustive selection of candidate member stars and dynamical study; and (v) the open clusters Berkeley 29 and Saurer 1, despite being located at large distances from the Galactic centre, are on nearly circular disc-like orbits. Conclusions. Even with our simple preliminary exploration of the Gaia EDR3, we demonstrate how, once again, these data from the European Space Agency are crucial for our understanding of the different pieces of our Galaxy and their connection to its global structure and history.

Item Type:

Article

Related URLs:

URL	URL Type	Description
https://doi.org/10.1051/0004-6361/202039714	DOI	Article
https://arxiv.org/abs/2101.05811	arXiv	Discussion Paper

ORCID:

Author	ORCID
Marocco, F.	0000-0001-7519-1700

Additional Information:

© ESO 2021. Article published by EDP Sciences. Received 19 October 2020; Accepted 12 January 2021; Published online 28 April 2021. We thank the referee Dr. James Binney for his comments. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This work presents results from the European Space Agency (ESA) space mission Gaia. Gaia data are being processed by the Gaia Data Processing and Analysis Consortium (DPAC). Funding for the DPAC is provided by national institutions, in particular the institutions participating in the Gaia MultiLateral Agreement (MLA). The Gaia mission website is https://www.cosmos.esa.int/gaia. The Gaia archive website is https://archives.esac.esa.int/gaia. The Gaia mission and data processing have financially been supported by, in alphabetical order by country: the Algerian Centre de Recherche en Astronomie,Astrophysique et Géophysique of Bouzareah Observatory; the Austrian Fonds zur Förderung der wissenschaftlichen Forschung (FWF) Hertha Firnberg Programme through grants T359, P20046, and P23737; the BELgian federal Science Policy Office (BELSPO) through various PROgramme de Développement d’Expériences scientifiques (PRODEX) grants and the Polish Academy of Sciences - Fonds Wetenschappelijk Onderzoek through grant VS.091.16N, and the Fonds de la Recherche Scientifique (FNRS); the Brazil-France exchange programmes Fundaçãode Amparo à Pesquisa do Estado de São Paulo (FAPESP) and Coordenação de Aperfeicoamento de Pessoal de Nível Superior (CAPES) - Comité Français d’Evaluation de la Coopération Universitaire et Scientifique avec le Brésil (COFECUB); the National Science Foundation of China (NSFC) through grants 11573054 and 11703065 and the China Scholarship Council through grant 201806040200; the Tenure Track Pilot Programme of the Croatian Science Foundation and the École Polytechnique Fédérale de Lausanne and the project TTP-2018-07-1171 ‘Mining the Variable Sky’, with the funds of the Croatian-Swiss Research Programme; the Czech-Republic Ministry of Education, Youth, and Sports through grant LG 15010 and INTER-EXCELLENCE grant LTAUSA18093, and the Czech Space Office through ESA PECS contract 98058; the Danish Ministry of Science; the Estonian Ministry of Education and Research through grant IUT40-1; the European Commission’s Sixth Framework Programme through the European Leadership in Space Astrometry (ELSA) Marie Curie Research Training Network (MRTN-CT-2006-033481), through Marie Curie project PIOF-GA-2009-255267 (Space AsteroSeismology and RR Lyrae stars, SAS-RRL), and through a Marie Curie Transfer-of-Knowledge (ToK) fellowship (MTKD-CT-2004-014188); the European Commission’s Seventh Framework Programme through grant FP7-606740 (FP7-SPACE-2013-1) for the Gaia European Network for Improved data User Services (GENIUS) and through grant 264895 for the Gaia Research for European Astronomy Training (GREAT-ITN) network; the European Research Council (ERC) through grants 320360 and 647208 and through the European Union’s Horizon 2020 research and innovation and excellent science programmes through Marie Skłodowska-Curie grant 745617 as well as grants 670519 (Mixing and Angular Momentum tranSport of massIvE stars – MAMSIE), 687378 (Small Bodies: Near and Far), 682115 (Using the Magellanic Clouds to Understand the Interaction of Galaxies), and 695099 (A sub-percent distance scale from binaries and Cepheids – CepBin); the European Science Foundation (ESF), in the framework of the Gaia Research for European Astronomy Training Research Network Programme (GREAT-ESF); the European Space Agency (ESA) in the framework of the Gaia project, through the Plan for European Cooperating States (PECS) programme through grants for Slovenia, through contracts C98090 and 4000106398/12/NL/KML for Hungary, and through contract 4000115263/15/NL/IB for Germany; the Academy of Finland and the Magnus Ehrnrooth Foundation; the French Centre National d’Etudes Spatiales (CNES), the Agence Nationale de la Recherche (ANR) through grant ANR-10-IDEX-0001-02 for the ‘Investissements d’avenir’ programme, through grant ANR-15-CE31-0007 for project ‘Modelling the Milky Way in the Gaia era’ (MOD4Gaia), through grant ANR-14-CE33-0014-01 for project ‘The Milky Way disc formation in the Gaia era’ (ARCHEOGAL), and through grant ANR-15-CE31-0012-01 for project ‘Unlocking the potential of Cepheids as primary distance calibrators’ (UnlockCepheids), the Centre National de la Recherche Scientifique (CNRS) and its SNO Gaia of the Institut des Sciences de l’Univers (INSU), the ‘Action Fédératrice Gaia’ of the Observatoire de Paris, the Région de Franche-Comté, and the Programme National de Gravitation, Références, Astronomie, et Métrologie (GRAM) of CNRS/INSU with the Institut National Polytechnique (INP) and the Institut National de Physique nucléaire et de Physique des Particules (IN2P3) co-funded by CNES; the German Aerospace Agency (Deutsches Zentrum für Luft- und Raumfahrt e.V., DLR) through grants 50QG0501, 50QG0601, 50QG0602, 50QG0701, 50QG0901, 50QG1001, 50QG1101, 50QG1401, 50QG1402, 50QG1403, 50QG1404, and 50QG1904 and the Centre for Information Services and High Performance Computing (ZIH) at the Technische Universität (TU) Dresden for generous allocations of computer time; the Hungarian Academy of Sciences through the Lendület Programme grants LP2014-17 and LP2018-7 and through the Premium Postdoctoral Research Programme (L. Molnár), and the Hungarian National Research, Development, and Innovation Office (NKFIH) through grant KH_18-130405; the Science Foundation Ireland (SFI) through a Royal Society – SFI University Research Fellowship (M. Fraser); the Israel Science Foundation (ISF) through grant 848/16; the Agenzia Spaziale Italiana (ASI) through contracts I/037/08/0, I/058/10/0, 2014-025-R.0, 2014-025-R.1.2015, and 2018-24-HH.0 to the Italian Istituto Nazionale di Astrofisica (INAF), contract 2014-049-R.0/1/2 to INAF for the Space Science Data Centre (SSDC, formerly known as the ASI Science Data Center, ASDC), contracts I/008/10/0, 2013/030/I.0, 2013-030-I.0.1-2015, and 2016-17-I.0 to the Aerospace Logistics Technology Engineering Company (ALTEC S.p.A.), INAF, and the Italian Ministry of Education, University, and Research (Ministero dell’Istruzione, dell’Università e della Ricerca) through the Premiale project ‘MIning The Cosmos Big Data and Innovative Italian Technology for Frontier Astrophysics and Cosmology’ (MITiC); the Netherlands Organisation for Scientific Research (NWO) through grant NWO-M-614.061.414, through a VICI grant (A. Helmi), and through a Spinoza prize (A. Helmi), and the Netherlands Research School for Astronomy (NOVA); the Polish National Science Centre through HARMONIA grant 2018/30/M/ST9/00311, DAINA grant 2017/27/L/ST9/03221, and PRELUDIUM grant 2017/25/N/ST9/01253, and the Ministry of Science and Higher Education (MNiSW) through grant DIR/WK/2018/12; the Portugese Fundação para a Ciência e a Tecnologia (FCT) through grants SFRH/BPD/74697/2010 and SFRH/BD/128840/2017 and the Strategic Programme UID/FIS/00099/2019 for CENTRA; the Slovenian Research Agency through grant P1-0188; the Spanish Ministry of Economy (MINECO/FEDER, UE) through grants ESP2016-80079-C2-1-R, ESP2016-80079-C2-2-R, RTI2018-095076-B-C21, RTI2018-095076-B-C22, BES-2016-078499, and BES-2017-083126 and the Juan de la Cierva formación 2015 grant FJCI-2015-2671, the Spanish Ministry of Education, Culture, and Sports through grant FPU16/03827, the Spanish Ministry of Science and Innovation (MICINN) through grant AYA2017-89841P for project ‘Estudio de las propiedades de los fósiles estelares en el entorno del Grupo Local’ and through grant TIN2015-65316-P for project ‘Computación de Altas Prestaciones VII’, the Severo Ochoa Centre of Excellence Programme of the Spanish Government through grant SEV2015-0493, the Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia ‘María de Maeztu’) through grants MDM-2014-0369 and CEX2019-000918-M, the University of Barcelona’s official doctoral programme for the development of an R+D+i project through an Ajuts de Personal Investigador en Formació (APIF) grant, the Spanish Virtual Observatory through project AyA2017-84089, the Galician Regional Government, Xunta de Galicia, through grants ED431B-2018/42 and ED481A-2019/155, support received from the Centro de Investigación en Tecnologías de la Información y las Comunicaciones (CITIC) funded by the Xunta de Galicia, the Xunta de Galicia and the Centros Singulares de Investigación de Galicia for the period 2016-2019 through CITIC, the European Union through the European Regional Development Fund (ERDF) / Fondo Europeo de Desenvolvemento Rexional (FEDER) for the Galicia 2014-2020 Programme through grant ED431G-2019/01, the Red Española de Supercomputación (RES) computer resources at MareNostrum, the Barcelona Supercomputing Centre - Centro Nacional de Supercomputación (BSC-CNS) through activities AECT-2016-1-0006, AECT-2016-2-0013, AECT-2016-3-0011, and AECT-2017-1-0020, the Departament d’Innovació, Universitats i Empresa de la Generalitat de Catalunya through grant 2014-SGR-1051 for project ‘Models de Programació i Entorns d’Execució Parallels’ (MPEXPAR), and Ramon y Cajal Fellowship RYC2018-025968-I; the Swedish National Space Agency (SNSA/Rymdstyrelsen); the Swiss State Secretariat for Education, Research, and Innovation through the ESA PRODEX programme, the Mesures d’Accompagnement, the Swiss Activités Nationales Complémentaires, and the Swiss National Science Foundation; the United Kingdom Particle Physics and Astronomy Research Council (PPARC), the United Kingdom Science and Technology Facilities Council (STFC), and the United Kingdom Space Agency (UKSA) through the following grants to the University of Bristol, the University of Cambridge, the University of Edinburgh, the University of Leicester, the Mullard Space Sciences Laboratory of University College London, and the United Kingdom Rutherford Appleton Laboratory (RAL): PP/D006511/1, PP/D006546/1, PP/D006570/1, ST/I000852/1, ST/J005045/1, ST/K00056X/1, ST/K000209/1, ST/K000756/1, ST/L006561/1, ST/N000595/1, ST/N000641/1, ST/N000978/1, ST/N001117/1, ST/S000089/1, ST/S000976/1, ST/S001123/1, ST/S001948/1, ST/S002103/1, and ST/V000969/1.

Group:

Infrared Processing and Analysis Center (IPAC)

Funders:

Funding Agency	Grant Number
Gaia Multilateral Agreement	UNSPECIFIED
Algerian Centre de Recherche en Astronomie	UNSPECIFIED
Astrophysique et Géophysique of Bouzareah Observatory	UNSPECIFIED
FWF Der Wissenschaftsfonds	T359
FWF Der Wissenschaftsfonds	P20046
FWF Der Wissenschaftsfonds	P23737
PROgramme de Développement d’Expériences scientifiques (PRODEX)	UNSPECIFIED
Polish Academy of Sciences	UNSPECIFIED
Fonds Wetenschappelijk Onderzoek (FWO)	VS.091.16N
Fonds de la Recherche Scientifique (FNRS)	UNSPECIFIED
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)	UNSPECIFIED
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)	UNSPECIFIED
Comité Français d’Évaluation de la Coopération Universitaire et Scientifique avec le Brésil (COFECUB)	UNSPECIFIED
National Natural Science Foundation of China	11573054
National Natural Science Foundation of China	11703065
China Scholarship Council	201806040200
Croatian Science Foundation	UNSPECIFIED
École Polytechnique Fédérale de Lausanne	UNSPECIFIED
Croatian-Swiss Research Programme	TTP-2018-07-1171
Ministry of Education, Youth, and Sports (Czech Republic)	LG 15010
Ministry of Education, Youth and Sports (MEYS) of the Czech Republic	LTAUSA18093
Czech Space Office	98058
Ministry of Higher Education and Science (Denmark)	UNSPECIFIED
Ministry of Education and Research (Estonia)	IUT40-1
Marie Curie Fellowship	MRTN-CT-2006-033481
Marie Curie Fellowship	PIOF-GA-2009-255267
Marie Curie Fellowship	MTKD-CT-2004-014188
European Research Council (ERC)	606740
European Research Council (ERC)	264895
European Research Council (ERC)	320360
European Research Council (ERC)	647208
Marie Curie Fellowship	745617
European Research Council (ERC)	670519
European Research Council (ERC)	687378
European Research Council (ERC)	682115
European Research Council (ERC)	695099
European Science Foundation	UNSPECIFIED
European Space Agency (ESA)	UNSPECIFIED
Plan for European Cooperating States (PECS)	C98090
Plan for European Cooperating States (PECS)	4000106398/12/NL/KML
Plan for European Cooperating States (PECS)	4000115263/15/NL/IB
Academy of Finland	UNSPECIFIED
Magnus Ehrnrooth Foundation	UNSPECIFIED
Centre National d’Études Spatiales (CNES)	UNSPECIFIED
Agence Nationale pour la Recherche (ANR)	ANR-10-IDEX-0001-02
Agence Nationale pour la Recherche (ANR)	ANR-15-CE31-0007
Agence Nationale pour la Recherche (ANR)	ANR-14-CE33-0014-01
Agence Nationale pour la Recherche (ANR)	ANR-15-CE31-0012-01
Centre National de la Recherche Scientifique (CNRS)	UNSPECIFIED
Institut national des sciences de l'Univers (INSU)	UNSPECIFIED
Observatoire de Paris	UNSPECIFIED
Région de Franche-Comté	UNSPECIFIED
Institut National Polytechnique (INP)	UNSPECIFIED
Institut National de Physique Nucléaire et de Physique des Particules (IN2P3)	UNSPECIFIED
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG0501
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG0601
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG0602
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG0701
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG0901
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1001
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1101
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1401
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1402
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1403
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1404
Deutsches Zentrum für Luft- und Raumfahrt (DLR)	50QG1904
Hungarian Academy of Sciences	LP2014-17
Hungarian Academy of Sciences	LP2018-7
National Research, Development, and Innovation Office (Hungary)	KH_18-130405
Science Foundation Ireland	UNSPECIFIED
Royal Society	UNSPECIFIED
Israel Science Foundation	848/16
Agenzia Spaziale Italiana (ASI)	I/037/08/0
Agenzia Spaziale Italiana (ASI)	I/058/10/0
Agenzia Spaziale Italiana (ASI)	2014-025-R.0
Agenzia Spaziale Italiana (ASI)	2014-025-R.1.2015
Agenzia Spaziale Italiana (ASI)	2018-24-HH.0
Istituto Nazionale di Astrofisica (INAF)	2014-049-R.0/1/2
Agenzia Spaziale Italiana (ASI)	I/008/10/0
Agenzia Spaziale Italiana (ASI)	2013/030/I.0
Agenzia Spaziale Italiana (ASI)	2013-030-I.0.1-2015
Agenzia Spaziale Italiana (ASI)	2016-17-I.0
Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR)	UNSPECIFIED
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)	NWO-M-614.061.414
Nederlandse Onderzoekschool Voor Astronomie (NOVA)	UNSPECIFIED
National Science Centre (Poland)	2018/06/M/ST9/00311
National Science Centre (Poland)	2017/27/L/ST9/03221
National Science Centre (Poland)	2017/25/N/ST9/01253
Ministerstwo Nauki i Szkolnictwa Wyższego (MNiSW)	DIR/WK/2018/12
Fundação para a Ciência e a Tecnologia (FCT)	SFRH/BPD/74697/2010
Fundação para a Ciência e a Tecnologia (FCT)	SFRH/BD/128840/2017
Fundação para a Ciência e a Tecnologia (FCT)	UID/FIS/00099/2019
Slovenian Research Agency	P1-0188
Ministerio de Economía, Industria y Competitividad (MINECO)	ESP2016-80079-C2-1-R
Ministerio de Economía, Industria y Competitividad (MINECO)	ESP2016-80079-C2-2-R
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Ministerio de Economía, Industria y Competitividad (MINECO)	BES-2016-078499
Ministerio de Economía, Industria y Competitividad (MINECO)	BES-2017-083126
Juan de la Cierva Fellowship	FJCI-2015-2671
Ministro de Educación, Cultura y Deporte (MECD)	FPU16/03827
Ministerio de Ciencia e Innovación (MCINN)	AYA2017-89841P
Ministerio de Ciencia e Innovación (MCINN)	TIN2015-65316-P
Centro de Excelencia Severo Ochoa	SEV2015-0493
Ministerio de Economía, Industria y Competitividad (MINECO)	MDM-2014-0369
Centro de Excelencia Severo Ochoa	CEX2019-000918-M
University of Barcelona	UNSPECIFIED
Ajuts de Personal Investigador en Formació (APIF)	UNSPECIFIED
Ministerio de Economía, Industria y Competitividad (MINECO)	AyA2017-84089
Xunta de Galicia	ED431B-2018/42
Xunta de Galicia	ED481A-2019/155
Centro de Investigación en Tecnologías de la Información y las Comunicaciones (CITIC)	UNSPECIFIED
Fondo Europeo de Desarrollo Regional (FEDER)	UNSPECIFIED
Xunta de Galicia	ED431G-2019/01
Red Española de Supercomputación (RES)	UNSPECIFIED
Barcelona Supercomputing Centre – Centro Nacional de Supercomputación (BSC-CNS)	AECT-2016-1-0006
Barcelona Supercomputing Centre – Centro Nacional de Supercomputación (BSC-CNS)	AECT-2016-2-0013
Barcelona Supercomputing Centre – Centro Nacional de Supercomputación (BSC-CNS)	AECT-2016-3-0011
Barcelona Supercomputing Centre – Centro Nacional de Supercomputación (BSC-CNS)	AECT-2017-1-0020
Generalitat de Catalunya	2014-SGR-1051
Ramón y Cajal Programme	RYC2018-025968-I
Swedish National Space Agency	UNSPECIFIED
State Secretariat for Education, Research, and Innovation (Switzerland)	UNSPECIFIED
Swiss Activités Nationales Complémentaires	UNSPECIFIED
Swiss National Science Foundation (SNSF)	UNSPECIFIED
Particle Physics and Astronomy Research Council (PPARC)	UNSPECIFIED
United Kingdom Space Agency (UKSA)	PP/D006511/1
United Kingdom Space Agency (UKSA)	PP/D006546/1
United Kingdom Space Agency (UKSA)	PP/D006570/1
Science and Technology Facilities Council (STFC)	ST/I000852/1
Science and Technology Facilities Council (STFC)	ST/J005045/1
Science and Technology Facilities Council (STFC)	ST/K00056X/1
Science and Technology Facilities Council (STFC)	ST/K000209/1
Science and Technology Facilities Council (STFC)	ST/K000756/1
Science and Technology Facilities Council (STFC)	ST/L006561/1
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Science and Technology Facilities Council (STFC)	ST/S000976/1
Science and Technology Facilities Council (STFC)	ST/S001123/1
Science and Technology Facilities Council (STFC)	ST/S001948/1
Science and Technology Facilities Council (STFC)	ST/S002103/1
Science and Technology Facilities Council (STFC)	ST/V000969/1

Subject Keywords:

Galaxy: disk – Galaxy: halo – stars: distances – open clusters and associations: individual: Saurer 1 – open clusters and associations: individual: Berkeley 29 – Galaxy: kinematics and dynamics

DOI:

10.1051/0004-6361/202039714

Record Number:

CaltechAUTHORS:20210510-070722783

Persistent URL:

https://resolver.caltech.edu/CaltechAUTHORS:20210510-070722783

Official Citation:

Gaia Early Data Release 3 - The Galactic anticentre Gaia Collaboration, T. Antoja, et. al., A&A, 649 (2021) A8; DOI: https://doi.org/10.1051/0004-6361/202039714

Usage Policy:

No commercial reproduction, distribution, display or performance rights in this work are provided.

ID Code:

109016

Collection:

CaltechAUTHORS

Deposited By:

Tony Diaz

Deposited On:

10 May 2021 20:25

Last Modified:

11 May 2021 15:03

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