{"paper":{"title":"The WFIRST Exoplanet Microlensing Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Aki Roberge, Andrea Belini, Andrew Cole, Aparna Bhattacharya, Arnaud Cassan, Atsunori Yonehara, Avi Mandell, Benjamin F. Williams, Bertrand Mennesson, Calen B. Henderson, Christian Coutures, Christopher Gelino, Clement Ranc, Daisuke Suzuki, David Ciardi, David Nataf, David P. Bennett, David Spergel, Dawn Gelino, Dominic J. Benford, Edward J. Wollack, Elisa Quintana, Etienne Bachelet, Ilaria Pascucci, James Rhodes, Jason D. Rhodes, Jason Kalirai, Jay Anderson, Jean-Phillipe Beaulieu, Jeffrey Kruk, Jennifer Yee, John Trauger, Jose A. Munoz, Joshua Schlieder, Kailash C. Sahu, Keith Horne, Keivan G. Stassun, Kenneth Carpenter, Kevin Grady, Knicole Colon, Lee Armus, Leonidas Moustakas, Leslie Rogers, Luigi Mancini, Martin Dominik, Matthew Penny, Maxime Rizzo, Michael McElwain, Michiel Lambrechts, Neil Zimmerman, Nicholas Rattenbury, N. Jeremy Kasdin, Padi Boyd, Pascal Fouque, Rachel Akeson, Rachel Street, Radek Poleski, Remi Soummer, Richard Barry, Roberta Paladini, Roeland van der Marel, Sangeeta Malhotra, Sara Seager, Sebastiano Calchi Novati, Seppo Laine, Shude Mao, Stephen Kane, Takahiro Sumi, Thomas Barclay, Tiffany Meshkat, Tyler Groff, Valerio Bozza, Vanessa Bailey, Yossi Shvartzvald","submitted_at":"2018-03-22T20:00:00Z","abstract_excerpt":"The Wide Field Infrared Survey Telescope (WFIRST) was the top ranked large space mission in the 2010 New Worlds, New Horizons decadal survey, and it was formed by merging the science programs of 3 different mission concepts, including the Microlensing Planet Finder (MPF) concept (Bennett \\etal\\ 2010). The WFIRST science program (Spergel \\etal\\ 2015) consists of a general observer program, a wavefront controlled technology program, and two targeted science programs: a program to study dark energy, and a statistical census of exoplanets with a microlensing survey, which uses nearly one quarter o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.08564","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":""},"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"}