{"paper":{"title":"Space VLBI 2020: Science and Technology Futures Conference Summary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"(10) Universit\\\"at zu K\\\"oln, (2) National Radio Astronomy Observatory, (3) California Institute of Technology, (4) Harvard-Smithsonian Center for Astrophysics, (5) Radboud University, (6) Graduate University of Advanced Studies, (7) Astro Space Center of Lebedev Physical Institute, (8) Massachusetts Institute of Technology/Haystack Observatory, (9) Shanghai Astronomical Observatory, Anthony J. Beasley (2) ( (1) Jet Propulsion Laboratory, Anton Zensus (10), California Institute of Technology, Colin J. Lonsdale (8), Heino Falcke (5), Katherine Bouman (3), Max-Planck-Institut fuer Radioastronomie), Moscow Institute of Physics & Technology, National Astronomical Observatory of Japan, Satoru Iguchi (6), Sheperd Doeleman (4), T. Joseph W. Lazio (1), Walter Brisken (2), Yuri Y. Kovalev (7), Zhiqiang Shen (9)","submitted_at":"2020-05-20T21:28:42Z","abstract_excerpt":"The \"Space VLBI 2020: Science and Technology Futures\" meeting was the second in The Future of High-Resolution Radio Interferometry in Space series. The first meeting (2018 September 5--6; Noordwijk, the Netherlands) focused on the full range of science applications possible for very long baseline interferometry (VLBI) with space-based antennas. Accordingly, the observing frequencies (wavelengths) considered ranged from below 1~MHz (> 300 m) to above 300~GHz (< 1 mm). For this second meeting, the focus was narrowed to mission concepts and the supporting technologies to enable the highest angula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2005.12767","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/2005.12767/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"}