{"paper":{"title":"Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A.G.G.M. Tielens, Akiko Kawamura, Akira Mizuno, Antonella Nota, Barbara Whitney, Bi-Qing For, Brian Babler, Charles W. Engelbracht, Ciska Markwick-Kemper, Claus Leitherer, Dennis Zaritsky, Douglas Kelly, Ed B. Churchwell, Francois Boulanger, Hiroshi Shibai, Jason Harris, Jay A. Frogel, Jay Gallagher, Jean-Philippe Bernard, Jeremy Mould, Joseph L. Hora, Karl D. Gordon, Karl Misselt, Kevin Volk, Knut Olsen, Linda Smith, Lister Staveley-Smith, Margaret Meixner, Marilyn Meade, Martin Cohen, Michael Werner, M.S. Oey, Nino Panagia, Norikazu Mizuno, Pablo Perez-Gonzalez, Remy Indebetouw, Roberta Paladini, Robert Blum, Sato Shuji, Schuyler Van Dyk, SoYoung Kim, Suzanne Madden, Toshikazu Onishi, Toshiya Ueta, Uma Vijh, Varoujan Gorjian, William B. Latter, William Reach, Yasuo Fukui","submitted_at":"2006-06-14T18:59:49Z","abstract_excerpt":"We are performing a uniform and unbiased, ~7x7 degrees imaging survey of the Large Magellanic Cloud (LMC), using the IRAC and MIPS instruments on board the Spitzer Space Telescope in order to survey the agents of a galaxy's evolution (SAGE), the interstellar medium (ISM) and stars in the LMC. The detection of diffuse ISM with column densities >1.2x10^21 H cm^-2 permits detailed studies of dust processes in the ISM. SAGE's point source sensitivity enables a complete census of newly formed stars with masses >3 solar masses that will determine the current star formation rate in the LMC. SAGE's de"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0606356","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0606356/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}