{"paper":{"title":"COSMOS-Web: An Overview of the JWST Cosmic Origins Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Ali Ahmad Khostovan, Alvio Renzini, Andreas L. Faisst, Angela Bongiorno, Anton M. Koekemoer, Arianna S. Long, Aristeidis Amvrosiadis, Bahram Mobasher, Behnam Darvish, Benny Trakhtenbrot, Brant E. Robertson, Brittany N. Vanderhoof, Caitlin M. Casey, Caitlin Rose, Christopher C. Hayward, Claudia Maraston, Clotilde Laigle, C. Megan Urry, Conor J. R. McPartland, Crystal L. Martin, Daizhong Liu, David B. Sanders, Diana Scognamiglio, Eleni Vardoulaki, Erini Lambrides, Fabrizio Gentile, Francesco Valentino, Gene C. K. Leung, Georgios Magdis, Ghassem Gozaliasl, Guillaume Mahler, Henry Joy McCracken, Hollis B. Akins, Isabella G. Cox, Jaclyn B. Champagne, Jacqueline E. McCleary, James W. Nightingale, Jason Rhodes, Jed McKinney, Jeyhan S. Kartaltepe, John D. Silverman, John R. Weaver, Jorge A. Zavala, Kartik Sheth, Katherine Chworowsky, Katherine E. Whitaker, Katriona M. L. Gould, Kevin C. Cooke, Knud Jahnke, Lilan Yang, Louise Paquereau, Margherita Talia, Marko Shuntov, Martin Sparre, Maximilien Franco, Micaela B. Bagley, Michaela Hirschmann, Nick Scoville, Nicole E. Drakos, Nima Chartab, Olivia R. Cooper, Olivier Ilbert, Oscar A. Chavez Ortiz, Peter L. Capak, Qiuhan He, Rafael C. Arango-Toro, Rebecca L. Larson, Richard Massey, R. Michael Rich, Rohan Pattnaik, Santosh Harish, Seiji Fujimoto, Shoubaneh Hemmati, Shuowen Jin, Sinclaire M. Manning, Stephen M. Wilkins, Steven Gillman, Steven L. Finkelstein, Sune Toft, Tobias Liaudat, Tomoko L. Suzuki, Vasily Kokorev, Vincenzo Mainieri, Xuheng Ding, Zahra Sattari","submitted_at":"2022-11-15T03:10:47Z","abstract_excerpt":"We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg$^2$ NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5$\\sigma$ point source depths ranging $\\sim$27.5-28.2 magnitudes. In parallel, we will obtain 0.19 deg$^2$ of MIRI imaging in one filter (F770W) reaching 5$\\sigma$ point source depths of $\\sim$25.3-26.0 magnitudes. COSMOS-Web will build on the rich heritage of multiwavelength observations a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.07865","kind":"arxiv","version":2},"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/2211.07865/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"}