{"paper":{"title":"Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Surveying the distant Universe","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"Alexander E. Thelen, Amelie Saintonge, Andreas Lundgren, Benjamin Magnelli, Carlos De Breuck, Chian-Chou Chen, Christopher C. Lovell, Claudia Cicone, Daizhong Liu, Doug Johnstone, Eelco van Kampen, Evanthia Hatziminaoglou, Francisco Miguel Montenegro-Montes, Helmut Dannerbauer, Juliette Hilhorst, Laura Sommovigo, Luca Di Mascolo, Mark Booth, Martin A. Cordiner, Matthew Smith, Matus Rybak, Minju Lee, Pamela Klaassen, Rob Ivison, Sven Wedemeyer, Sy-Yun Pu, Teppei Okumura, Thomas J. Maccarone, Tom Bakx, Tony Mroczkowski","submitted_at":"2024-03-05T09:22:30Z","abstract_excerpt":"During the most active period of star formation in galaxies, which occurs in the redshift range 1<z<3, strong bursts of star formation result in significant quantities of dust, which obscures new stars being formed as their UV/optical light is absorbed and then re-emitted in the infrared, which redshifts into the mm/sub-mm bands for these early times. To get a complete picture of the high-z galaxy population, we need to survey a large patch of the sky in the sub-mm with sufficient angular resolution to resolve all galaxies, but we also need the depth to fully sample their cosmic evolution, and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.02806","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/2403.02806/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"}