{"paper":{"title":"Detailed cool star flare morphology with CHEOPS and TESS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"A. Boldog, A. Brandeker, A. Collier Cameron, A. Deline, A. Erikson, A.E. Simon, A. Fortier, A. Heitzmann, A. Lecavelier des Etangs, A.M.S. Smith, B.-O. Demory, B. Ulmer, C. Broeg, Ch. Helling, C. Mordasini, D. Barrado Navascues, D. Ehrenreich, D. Gandolfi, D. Magrin, D. Pollacco, D. Queloz, D. S\\'egransan, E. Pall\\'e, E. Villaver, F. Ratti, G. Bruno, G. Olofsson, G. Peter, G. Piotto, G. Scandariato, H.-G. Flor\\'en, H. Rauer, I. Pagano, I. Ribas, J. Farinato, J. Laskar, J. Venturini, K.G. Isaak, K.W.F. Lam, L. Borsato, L. Delrez, L. Fossati, L. Kiss, L. Kriskovics, M.B. Davies, M. Beck, M. Deleuil, M. Fridlund, M. Gillon, M. G\\\"udel, M. Gy. Szab\\'o, M. Lendl, M.N. G\\\"unther, M. Sarajlic, M. Stalport, N.A. Walton, N. Billot, N.C. Santos, N. Rando, N. Thomas, O.D.S. Demangeon, P.E. Cubillos, P.F.L. Maxted, R. Alonso, R. Ottensamer, R. Ragazzoni, S.C.C. Barros, S.G. Sousa, S. Hoyer, S. Sulis, S. Udry, Sz. Csizmadia, T. B\\'arczy, T. Beck, T.G. Wilson, V. Nascimbeni, V. Singh, V. Van Grootel, W. Baumjohann, W. Benz, Y. Alibert, Z. Garai","submitted_at":"2024-03-25T18:00:54Z","abstract_excerpt":"Context. White-light stellar flares are proxies for some of the most energetic types of flares, but their triggering mechanism is still poorly understood. As they are associated with strong X and UV emission, their study is particularly relevant to estimate the amount of high-energy irradiation onto the atmospheres of exoplanets, especially those in their stars' habitable zone. Aims. We used the high-cadence, high-photometric capabilities of the CHEOPS and TESS space telescopes to study the detailed morphology of white-light flares occurring in a sample of 130 late-K and M stars, and compared "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.17065","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/2403.17065/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"}