{"paper":{"title":"The EBLM project -- IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"A. Brandeker, A. Collier Cameron, A. Erikson, A. E. Simon, A. Fortier, A. H. M. J. Triaud, A. Lecavelier des Etangs, A. M. S. Smith, A. Santerne, B.-O. Demory, C. Broeg, C. Lovis, C. M. Persson, D. Barrado, D. Ehrenreich, D. Gandolfi, D. Magrin, D. Pollacco, D. Queloz, D. Sebastian, D. S\\'egransan, D. V. Martin, E. Kopp, E. Pall\\'e, F. A. Pepe, G. Anglada, G. Dransfield, G. H\\'ebrard, G. Olofsson, G. Peter, G. Piotto, G. Scandariato, Gy. M. Szab\\'o, H. Rauer, I. Boisse, I. Pagano, I. Ribas, J. Asquier, J. Cabrera, J. Hasiba, J. Laskar, J. McCormac, K. G. Isaak, K. Heng, L. Delrez, L. Fossati, L. L. Kiss, M. B. Davies, M. Beck, M. Bergomi, M. Deleuil, M. Fridlund, M. Gillon, M. G\\\"udel, M. I. Swayne, M. Lendl, M. P. Battley, M. R. Standing, M. Steller, N. A. Walton, N. Billot, N. C. Santos, N. Heidari, N. J. Miller, N. Rando, N. Thomas, O. D. S. Demangeon, P. F. L. Maxted, R. Alonso, R. Ottensamer, R. Ragazzoni, S. C. C. Barros, S. Charnoz, S. Gill, S. G. Sousa, S. Hoyer, S. Lalitha, S. Udry, Sz. Csizmadia, T. B\\'arczy, T. Beck, V. Kunovac, V. Nascimbeni, V. Van Grootel, W. Baumjohann, W. Benz, X. Bonfils, Y. Alibert","submitted_at":"2022-09-07T13:28:44Z","abstract_excerpt":"Eclipsing binaries are important benchmark objects to test and calibrate stellar structure and evolution models. This is especially true for binaries with a fully convective M-dwarf component for which direct measurements of these stars' masses and radii are difficult using other techniques. Within the potential of M-dwarfs to be exoplanet host stars, the accuracy of theoretical predictions of their radius and effective temperature as a function of their mass is an active topic of discussion. Not only the parameters of transiting exoplanets but also the success of future atmospheric characteri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.03128","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/2209.03128/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"}