{"paper":{"title":"Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Alexander van Engelen, An\\v{z}e Slosar, Benjamin Beringue, Benjamin Rose, Benjamin Saliwanchik, Bhuvnesh Jain, Bradford Benson, Bradley Johnson, Bruce Partridge, Carlo Baccigalupi, Christopher M. Hirata, Cora Dvorkin, Daan Meerburg, Daisuke Nagai, Darcy Barron, David Frayer, David N. Spergel, Dongwon Han, Ely D. Kovetz, Emmanuel Schaan, Eric Baxter, Eric R. Switzer, Erminia Calabrese, Erwin T. Lau, Evan B. Grohs, Florian Beutler, Francesco Piacentni, Francis-Yan Cyr-Racine, George M. Fuller, Gil Holder, Graziano Rossi, Ho Nam Nguyen, Huanyuan Shan, Hy Trac, J. Colin Hill, Joel Meyers, J. Richard Bond, Julian Borrill, Kaustuv Basu, Kelly A. Douglass, Laura Newburgh, Luca Di Mascolo, Marc Kamionkowski, Martina Gerbino, Mathew Madhavacheril, Matias Zaldarriaga, Matthew C. Johnson, Michael Zemcov, Michele Liguori, Moritz Munchmeyer, Neelima Sehgal, Nikhel Gupta, Omar Darwish, Pamela Klaassen, Pavel Motloch, Peter Adshead, Robert Armstrong, Sara Simon, Satya Gontcho A Gontcho, Selim Hotinli, Simon Dicker, Simone Ferraro, Simon Foreman, S. Lucas Denny, Tom Essinger-Hileman, Tony Mroczkowski, Toshiya Namikawa, Vera Gluscevic, Weishuang Xu","submitted_at":"2019-03-08T03:21:37Z","abstract_excerpt":"Opening up a new window of millimeter-wave observations that span frequency bands in the range of 30 to 500 GHz, survey half the sky, and are both an order of magnitude deeper (about 0.5 uK-arcmin) and of higher-resolution (about 10 arcseconds) than currently funded surveys would yield an enormous gain in understanding of both fundamental physics and astrophysics. In particular, such a survey would allow for major advances in measuring the distribution of dark matter and gas on small-scales, and yield needed insight on 1.) dark matter particle properties, 2.) the evolution of gas and galaxies,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.03263","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"}