{"paper":{"title":"HAT-P-39b--HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bieryla, A. Shporer, A. W. Howard, B. B\\'eky, B. J. Fulton, D. A. Fischer, D. D. Sasselov, D. W. Latham, G.\\'A. Bakos, G. A. Esquerdo, G. F\\H{u}r\\'esz, G. Kov\\'acs, G. Torres, G. W. Marcy, I. Papp, J. A. Johnson, J. D. Hartman, J. L\\'az\\'ar, K. Penev, L. A. Buchhave, M. Everett, P. Hinz, P. S\\'ari, R. P. Knox, R. P. Stefanik, R. W. Noyes, S. N. Quinn, T. Szklen\\'ar, Z. Csubry","submitted_at":"2012-07-13T19:58:11Z","abstract_excerpt":"We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V=11.1 to 12.4) F stars. The planets have periods of P = 2.6940 d to 4.4572 d, masses of 0.60 M_J to 0.80 M_J, and radii of 1.57 R_J to 1.73 R_J. They orbit stars with masses between 1.40 M_sun and 1.51 M_sun. The three planets are members of an emerging population of highly inflated Jupiters with 0.4 M_J < M < 1.5 M_J and R > 1.5 R_J."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.3344","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"}