{"paper":{"title":"Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"(10) University of California, (11) NASA Exoplanet Science Institute/Caltech, (12) Jet Propulsion Laboratory/California Institute of Technology, (13) Carnegie Institution of Washington, (14) Niels Bohr Institute, 15), (15) Centre for Star, (16) Aarhus University, (17) McDonald Observatory, (18) Department of Earth, (19) SETI Institute, (20) National Optical Astronomy Observatory, (21) Orbital Sciences Corporation/NASA Ames Research Center, (22) Lawrence Hall of Science, (23) Centre for Astrophysics, (24) Villanova University, (25) Fermilab Center for Particle Astrophysics, (26) Bay Area Environmental Research Institute/NASA Ames Research Center, (27) Department of Astrophysical Sciences, (28) San Diego State University, 29), (29) Department of Physics, (2) SETI Institute/NASA Ames Research Center, (3) NASA Ames Research Center, (4) Bay Area Environmental Research Institute/NASA Ames Research Center, (5) Las Cumbres Observatory Global Telescope Network, (6) Harvard-Smithsonian Center for Astrophysics, (7) Department of Astronomy, (8) University of Florida, (9) Center for Exoplanets, Alan Gould (22), Alan P. Boss (13), Andrea K. Dupree (6), Andrej Prsa (24), Andrew W. Howard (10), Astronomy, Astrophysics, Atmospheric, Avi Shporer (5), Berkeley, Brice-Olivier Demory (18), Bruce D. Clarke (12), Christopher J. Burke (2), Daniel C. Fabrycky (7), Darin Ragozzine (6), David Charbonneau (6), David G. Koch (3), David R. Ciardi (11), David W. Latham (6), Dimitar Sasselov (6), Douglas A. Caldwell (2), Dwight T. Sanderfer (21), Edna Devore (19), Elisa Quintana (2), Eric B. Ford (8), Fergal Mullally (2), Forrest R. Girouard (21), Francois Fressin (6), Geoffrey W. Marcy (10), Georgia State University), Gibor S. Basri (10), Gilbert A. Esquerdo (6), Guillermo Torres (6), Habitable Worlds, Hans Kjeldsen (16), Howard Isaacson (10), Jack J. Lissauer (3), Jason F. Rowe (2), Jason H. Steffen (25) Martin Still (26), Jeffrey C. Smith (2), Jeffrey Van Cleve (2), Jennifer R. Hall (21), Jessie L. Christiansen (3), Jie Li (2), Jill C. Tarter (19), Joergen Christensen-Dalsgaard (16), John C. Geary (6), Jonathan J. Fortney (7), Jon M. Jenkins (2), Joseph D. Twicken (2), Kamal Uddin (21), Khadeejah A. Ibrahim (21), K. Kinemuchi (2), Lars A. Buchhave (14, Lucianne Walkowicz (27), Mark Everett (20), Martin C. Stumpe (2), Massachusetts Institute of Technology, Matthew J. Holman (6), Michael R. Haas (3), Natalie M. Batalha (1), Natural History Museum of Denmark, Peter Tenenbaum (2), Philip W. Lucas (23), Planetary Sciences, Planet Formation, Princeton University, Robert L. Morris (21), Ronald L. Gilliland (9), Samuel Quinn (6, San Jose State University, Shawn E. Seader (2), Stephen T. Bryson (3), Steve B. Howell (3), Susan E. Thompson (2), The Pennsylvania State University, The University of Texas, Thomas Barclay (4), Thomas N. Gautier III (12), Timothy M. Brown (5), Todd C. Klaus (21), University of California, University of Copenhagen, University of Hertfordshire, William D. Cochran (17), William F. Welsh (28) ((1) Department of Physics, William J. Borucki (3), William Rapin (3)","submitted_at":"2012-02-27T08:34:01Z","abstract_excerpt":"New transiting planet candidates are identified in sixteen months (May 2009 - September 2010) of data from the Kepler spacecraft. Nearly five thousand periodic transit-like signals are vetted against astrophysical and instrumental false positives yielding 1,091 viable new planet candidates, bringing the total count up to over 2,300. Improved vetting metrics are employed, contributing to higher catalog reliability. Most notable is the noise-weighted robust averaging of multi-quarter photo-center offsets derived from difference image analysis which identifies likely background eclipsing binaries"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.5852","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"}