{"paper":{"title":"Characterisation of the Warm-Jupiter TOI-1130 system with CHEOPS and photo-dynamical approach","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Bekkelien, A. Bonfanti, A. Brandeker, A.C.M. Correia, A. Collier Cameron, A. Deline, A. Derekas, A. Erikson, A.E. Simon, A. Fortier, A. Heitzmann, A.H.M.J. Triaud, A. Lecavelier des Etangs, A. Leleu, A.M. S. Smith, B. Edwards, B.-O. Demory, C. Broeg, Ch. Helling, C. Mordasini, C.M. Persson, D. Barrado Navascues, D. Degen, D. Ehrenreich, D. Gandolfi, D. Magrin, D. M\\'ekarnia, D. Mura, D. Pollacco, D. Queloz, D. S\\'egransan, D. Wolter, E. Pall\\'e, E. Villaver, F. Ratti, G. Olofsson, G. Peter, G. Piotto, G. Scandariato, Gy.M. Szab\\'o, H. Rauer, I. Pagano, I. Ribas, J.A. Egger, J. Korth, J. Laskar, J. Venturini, K. Gazeas, K.G. Isaak, K.W.F. Lam, L. Abe, L. Borsato, L. Delrez, L. Fossati, L.L. Kiss, L. Marafatto, M.B. Davies, M.-D. Busch, M. Deleuil, M. Fridlund, M. Gillon, M. G\\\"udel, M.J. Hooton, M. Lendl, M. Mecina, M.N. G\\\"unther, M. Stalport, N.A. Walton, N. Billot, N.C. Santos, N. Rando, O.D. S. Demangeon, O. Suarez, P. Bendjoya, P.E. Cubillos, P.F.L. Maxted, R. Alonso, R. Ottensamer, R. Ragazzoni, S.C. C. Barros, S.G. Sousa, S. Hoyer, S. Salmon, S. Sulis, S. Udry, Sz. Csizmadia, T. B\\'arczy, T. Beck, T. Guillot, T.G. Wilson, T. Zingales, V. Nascimbeni, V. Van Grootel, W. Baumjohann, W. Benz, Y. Alibert","submitted_at":"2024-07-08T16:37:52Z","abstract_excerpt":"Among the thousands of exoplanets discovered to date, approximately a few hundred gas giants on short-period orbits are classified as \"lonely\" and only a few are in a multi-planet system with a smaller companion on a close orbit. The processes that formed multi-planet systems hosting gas giants on close orbits are poorly understood, and only a few examples of this kind of system have been observed and well characterised. Within the contest of multi-planet system hosting gas-giant on short orbits, we characterise TOI-1130 system by measuring masses and orbital parameters. This is a 2-transiting"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.06097","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/2407.06097/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"}