{"paper":{"title":"Three Hot Jupiters transiting K-dwarfs with a significant heavy element mass","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Popowicz, A. Revol, A.W. Mann, B. Lavie, B. Tofflemire, C. Farret Jentink, C. Hellier, C.N. Watkins, C. Ziegler, D.J. Radford, D.W. Latham, E. Fontanet, E. Frid\\'en, E. Jehin, E. Palle, F. Bouchy, F.J. Pozuelos, F. Murgas, F. Pepe, G. Furesz, G. Lo Curto, G. Ricker, H. Chakraborty, H.M. Relles, I.A. Strakhov, J.M. Jenkins, J.N. Winn, J.P. Faria, K.A. Collins, K. Barkaoui, K.G. Stassun, L.K.W. Kwok, L. Parc, M. Battley, M. Gillon, M. Shinde, M. Steiner, M. Timmermans, N.C. Santos, N. Grieves, N. Law, P. Evans, R. Vanderspek, S.G. Sousa, S. Seager, S. Tavella, S. Udry, S. Ulmer-Moll, T. Daylan, T.-G. Tan, V. Vaulato, W. Ceva, Y.G.C. Frensch","submitted_at":"2025-06-05T11:56:30Z","abstract_excerpt":"Albeit at a lower frequency than around hotter stars, short-period gas giants around low-mass stars ($T_\\mathrm{eff} < 4965$ K) do exist, despite predictions from planetary population synthesis models that such systems should be exceedingly rare. By combining data from TESS and ground-based follow-up observations, we seek to confirm and characterize giant planets transiting K dwarfs, particularly mid/late K dwarfs. Photometric data were obtained from the TESS mission, supplemented by ground-based imaging- and photometric observations, as well as high-resolution spectroscopic data from the CORA"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.04923","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/2506.04923/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"}