{"paper":{"title":"EPIC247098361b: a transiting warm Saturn on an eccentric $P=11.2$ days orbit around a $V=9.9$ star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Andr\\'es Jord\\'an, Blake Pantoja, Felipe Rojas, Holger Drass, James J. Jenkins, Maja V\\v{u}ckovi\\'c, Maritza G. Soto, Markus Rabus, Mat\\'ias I. Jones, Mat\\'ias R. D\\'iaz, N\\'estor Espinoza, Paula Sarkis, Rafael Brahm, R\\'egis Lachaume, Thomas Henning","submitted_at":"2018-02-24T15:38:23Z","abstract_excerpt":"We report the discovery of EPIC247098361b using photometric data of the Kepler K2 satellite coupled with ground-based spectroscopic observations. EPIC247098361b has a mass of M$_{P}=0.397\\pm 0.037$ M$_J$, a radius of R$_{P}=1.00 \\pm 0.020$ R$_J$, and a moderately low equilibrium temperature of $T_{eq}=1030 \\pm 15$ K due to its relatively large star-planet separation of $a=0.1036$ AU. EPIC247098361b orbits its bright ($V=9.9$) late F-type host star in an eccentric orbit ($e=0.258 \\pm 0.025$) every 11.2 days, and is one of only four well characterized warm Jupiters having hosts stars brighter th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.08865","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"}