{"paper":{"title":"Near-resonance in a system of sub-Neptunes from TESS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Ana Glidden, Andrei Tokovinin, Andrew Vanderburg, Andrew W. Mann, Artem Burdanov, Avi Shporer, Carl Ziegler, Catriona Murray, Charles A. Beichman, Chelsea X. Huang, Damien S\\'egransan, Daniel Sebastian, David Armstrong, David Charbonneau, David Ciardi, David W. Latham, Dennis M. Conti, Diana Dragomir, Elisabeth Matthews, Elliott P. Horch, Elsa Ducrot, Emmanuel Jehin, Enric Palle, Eric Agol, Erica J. Gonzales, Eric L. N. Jensen, Felipe Murgas, Fran\\c{c}ois Bouchy, Francesco Pepe, Francisco J. Pozuelos, Fred Adams, Ga\\\"el Ottoni, George R. Ricker, Howard M. Relles, Ian J. M. Crossfield, Ian Waite, Jack J. Lissauer, Jason D. Eastman, Jason Dittmann, Jennifer Campbell, Jerome Pitogo de Leon, Jessie L. Christiansen, John Doty, John F. Kielkopf, Jonathan Horner, Jon M. Jenkins, Joseph D. Twicken, Joseph E. Rodriguez, Joshua E. Schlieder, Joshua N. Winn, Juliette C. Becker, Karen A. Collins, Keivan G. Stassun, Kevin I. Collins, Khalid Barkaoui, Krzysztof G. He{\\l}miniak, L. G. Bouma, Louise D. Nielsen, Martti H. Kristiansen, Maxime Marmier, Mayuko Mori, Michael Gillon, Motohide Tamura, Nicholas Law, Norio Narita, Rachel A. Matson, Rafa{\\l} Paw{\\l}aszek, Robert F. Goeke, Roberto Carlino, Rob Wittenmyer, Roland K. Vanderspek, Sam Hadden, Samuel N. Quinn, Sara Seager, Scott M. Cartwright, St\\'ephane Udry, Stephen R. Kane, Steve B. Howell, Tansu Daylan, Timothy D. Morton, Tsevi Mazeh","submitted_at":"2019-01-25T21:40:57Z","abstract_excerpt":"We report the Transiting Exoplanet Survey Satellite ($TESS$) detection of a multi-planet system orbiting the $V=10.9$ K0 dwarf TOI 125. We find evidence for up to five planets, with varying confidence. Three high signal-to-noise transit signals correspond to sub-Neptune-sized planets ($2.76$, $2.79$, and $2.94\\ R_{\\oplus}$), and we statistically validate the planetary nature of the two inner planets ($P_b = 4.65$ days, $P_c = 9.15$ days). With only two transits observed, we report the outer object ($P_{.03} = 19.98$ days) as a high signal-to-noise ratio planet candidate. We also detect a candi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.09092","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/1901.09092/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"}