{"paper":{"title":"PLATO as it is: a legacy mission for Galactic archaeology","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. Bressan, A. Miglio, A. Noels, A. Recio-Blanco, A. Robin, A. Serenelli, B. Barbuy, B. Famaey, B. Holl, B. K. Gibson, B. Mosser, B. M. Rendle, B. Plez, B. X. Santiago, C. Allende Prieto, C. Babusiaux, C. Barban, C. Cacciari, C. Chiappini, C.C. Worley, C. Reyle, C. Soubiran, D. Bossini, D. Huber, D. Katz, D. Kawata, D. Pollacco, D. Pricopi, D. Stello, D.W. Kurtz, E.Depagne, F. Anders, F. Baudin, F. Combes, G. Gilmore, G. Piotto, G.R. Davies, H. Kjeldsen, H. Rauer, I. Minchev, I. W. Roxburgh, J. Binney, J. Bland-Hawthorn, J. Christensen-Dalsgaard, J.DeRidder, J. Montalban, K. Belkacem, K. Brogaard, K. Freeman, K.G. Strassmeier, K. Hawkins, L. Casagrande, L. Girardi, L. Gizon, M.-A. Dupret, M. Haywood, M.H. Pinsonneault, M.-J. Goupil, M. Martig, M.N. Lund, M.P.Di Mauro, M. Salaris, M.S. Cunha, M. Steinmetz, M. Valentini, N. A. Walton, N. Lagarde, O. Benomar, O. Bienayme, O. Creevey, O. Gerhard, P. de Laverny, P.DiMatteo, P. Eggenberger, P.G. Prada Moroni, P. Jofre, P. Marigo, P.P. Avelino, P.Ventura, R. A. Garcia, R. Handberg, R. Ibata, R. Schiavon, R.S. de Jong, R.Ventura, S. Basu, S. Cassisi, S.Degl'Innocenti, S.Deheuvels, S.D. Kawaler, S. Feltzing, S. Hekker, S. Mathur, S. Ortolani, S.R. Majewski, S. Sharma, T. Appourchaux, T.L. Campante, T. Morel, T. Rodrigues, U. Heiter, V. Silva Aguirre, W. J. Chaplin, Y. Elsworth, Y. Lebreton","submitted_at":"2017-06-12T18:00:03Z","abstract_excerpt":"Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy. Data from large-scale astrometric and spectroscopic surveys will soon provide us with a well-defined view of the current chemo-kinematical structure of the Milky Way, but will only enable a blurred view on the temporal sequence that led to the present-day Galaxy. As demonstrated by the (ongoing) exploitation of data from the pioneering photometric missions CoRoT, Kepler, and K2, asteroseismology provides the way forw"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.03778","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}