{"paper":{"title":"Maximizing Science in the Era of LSST: A Community-Based Study of Needed US Capabilities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Adam Bolton (NOAO), Alex Drlica-Wagner (Fermilab), Anja von der Linden (SUNY), Beth Willman (LSST), Branimir Sesar (Max Planck Institute for Astronomy), Bryan W. Miller (Gemini Observatory), Caltech), Chad Schafer (Carnegie Mellon U.), Constance M. Rockosi (UC Santa Cruz), Cristina A. Thomas (Planetary Science Institute), David Ciardi (IPAC, David J. Sand (Texas Tech U.), David Trilling (Northern Arizona U.), Dawn Erb (U. Wisconsin-Milwaukee), Derek Buzasi (Florida Gulf Coast U.), Douglas P. Finkbeiner (Harvard University), Elise Jennings (Fermilab), Eric F. Bell (U. Michigan), Eric Gawiser (Rutgers), Eric Linder (LBNL), Erik J. Tollerud (STScI), Gregory Rudnick (U. Kansas), Henry Hsieh (Planetary Science Institute), James R. A. Davenport (Western Washington U.), Jay Elias (NOAO), Jeffrey A. Newman (U. Pittsburgh), Jennifer L. Hoffman (U. Denver), Joan Najita (NOAO), John O'Meara (Saint Michael's College), Jon Trump (Penn State U.), Joshua D. Simon (Carnegie Observatories), Kathryn V. Johnston (Columbia U.), Lori Feaga (U. Maryland), Mark Dickinson (NOAO), Mark Giampapa (NSO), Phil Marshall (SLAC National Accelerator Laboratory), Puragra Guhathakurta (UC Santa Cruz), Rachel Mandelbaum (Carnegie Mellon U.), Rachel Street (LCOGT), Ruth Angus (U. Oxford), Ryan J. Foley (UC Santa Cruz), Sam Schmidt (UC Davis), Scott S. Sheppard (Carnegie Institute for Science/Department of Terrestrial Magnetism), Soren Meibom (Harvard-Smithsonian CfA), Steve Ridgway (NOAO), Suzanne Hawley (U. Washington), Thomas Matheson (NOAO), Ting S. Li (Texas A&M University), Vinay Kashyap (Harvard-Smithsonian CfA), Vishnu Reddy (U. Arizona), Wen-fai Fong (U. Arizona), Will Dawson (LLNL)","submitted_at":"2016-10-05T21:37:17Z","abstract_excerpt":"The Large Synoptic Survey Telescope (LSST) will be a discovery machine for the astronomy and physics communities, revealing astrophysical phenomena from the Solar System to the outer reaches of the observable Universe. While many discoveries will be made using LSST data alone, taking full scientific advantage of LSST will require ground-based optical-infrared (OIR) supporting capabilities, e.g., observing time on telescopes, instrumentation, computing resources, and other infrastructure. This community-based study identifies, from a science-driven perspective, capabilities that are needed to m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.01661","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"}