{"paper":{"title":"TTV-determined Masses for Warm Jupiters and their Close Planetary Companions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Dong-Hong Wu, Gregory Laughlin, Jason H. Steffen, Ji-Lin Zhou, Songhu Wang","submitted_at":"2018-07-06T01:37:51Z","abstract_excerpt":"Although the formation and the properties of hot Jupiters (with orbital periods $P<10\\,$d) have attracted a great deal of attention, the origins of warm Jupiters ($10<P<100\\,$d) are less well-studied. Using a transit timing analysis, we present the orbital parameters of five planetary systems containing warm Jupiters, Kepler 30, Kepler 117, Kepler 302, Kepler 487 and Kepler 418. Three of them, Kepler-30 c($M_p=549.4{\\pm{5.6}}M_{\\oplus}$), Kepler-117 c($M_p=702{\\pm{63}}M_{\\oplus}$) and Kepler 302 c($M_p=933\\pm 527M_{\\oplus}$), are confirmed to be real warm Jupiters based on their mass. Insights"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.02217","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"}