{"paper":{"title":"Stellar archaeology with Gaia: the Galactic white dwarf population","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Alina Istrate, Anna Pala, Boris Gaensicke, Christian Knigge, Christopher Manser, David Wilson, Dimitri Veras, Enrique Garcia-Berro, Gijs Nelemans, Giuseppe Bono, Jay Farihi, JJ Hermes, Klaus Werner, Mark Hollands, Martin Barstow, Matt Burleigh, Nicola Gentile-Fusillo, Odette Toloza, Pier-Emmanuel Tremblay, Roberto Raddi, Sarah Casewell, Stefan Jordan, Stephan Geier, Thomas Tauris, Tom Marsh, Vik Dhillon","submitted_at":"2015-06-08T20:00:21Z","abstract_excerpt":"Gaia will identify several 1e5 white dwarfs, most of which will be in the solar neighborhood at distances of a few hundred parsecs. Ground-based optical follow-up spectroscopy of this sample of stellar remnants is essential to unlock the enormous scientific potential it holds for our understanding of stellar evolution, and the Galactic formation history of both stars and planets."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.02653","kind":"arxiv","version":1},"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"}