Exploiting timing capabilities of the CHEOPS mission with warm-Jupiter planets

Autor: L, Borsato, G, Piotto, D, Gandolfi, V, Nascimbeni, G, Lacedelli, F, Marzari, N, Billot, P, Maxted, G, Sousa S, C, Cameron A, A, Bonfanti, T, Wilson, L, Serrano, Z, Garai, Y, Alibert, R, Alonso, J, Asquier, T, Bárczy, T, Bandy, D, Barrado, C, Barros S, W, Baumjohann, M, Beck, T, Beck, W, Benz, X, Bonfils, A, Brandeker, C, Broeg, J, Cabrera, S, Charnoz, S, Csizmadia, M, Davies, M, Deleuil, L, Delrez, D, Demangeon O, B, Demory, A, Lecavelier des Etangs, D, Ehrenreich, A, Erikson, G, Escudé, A, Fortier, L, Fossati, M, Fridlund, M, Gillon, M, Guedel, J, Hasiba, K, Heng, S, Hoyer, G, Isaak K, L, Kiss L, E, Kopp, J, Laskar, M, Lendl, C, Lovis, D, Magrin, M, Munari, R, Ottensamer, G, Peter, R, Ragazzoni, N, Rando, E, Simon A, M, Steller, G, Olofsson, I, Pagano, E, Palle, D, Pollacco, D, Queloz, H, Rauer, I, Ribas, D, Segransan, M, Santos N, G, Scandariato, A, Smith, M, Szabo G, N, Thomas, S, Udry, Grootel V, Van, A, Walton N

We present 17 transit light curves of seven known warm-Jupiters observed with the CHaracterising ExOPlanet Satellite (CHEOPS). The light curves have been collected as part of the CHEOPS Guaranteed Time Observation (GTO) program that searches for tran

Externí odkaz: http://arxiv.org/abs/2106.11331

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The EBLM project – IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves

Autor: D Sebastian, M I Swayne, P F L Maxted, A H M J Triaud, S G Sousa, G Olofsson, M Beck, N Billot, S Hoyer, S Gill, N Heidari, D V Martin, C M Persson, M R Standing, Y Alibert, R Alonso, G Anglada, J Asquier, T Bárczy, D Barrado, S C C Barros, M P Battley, W Baumjohann, T Beck, W Benz, M Bergomi, I Boisse, X Bonfils, A Brandeker, C Broeg, J Cabrera, S Charnoz, A Collier Cameron, Sz Csizmadia, M B Davies, M Deleuil, L Delrez, O D S Demangeon, B-O Demory, G Dransfield, D Ehrenreich, A Erikson, A Fortier, L Fossati, M Fridlund, D Gandolfi, M Gillon, M Güdel, J Hasiba, G Hébrard, K Heng, K G Isaak, L L Kiss, E Kopp, V Kunovac, J Laskar, A Lecavelier des Etangs, M Lendl, C Lovis, D Magrin, J McCormac, N J Miller, V Nascimbeni, R Ottensamer, I Pagano, E Pallé, F A Pepe, G Peter, G Piotto, D Pollacco, D Queloz, R Ragazzoni, N Rando, H Rauer, I Ribas, S Lalitha, A Santerne, N C Santos, G Scandariato, D Ségransan, A E Simon, A M S Smith, M Steller, Gy M Szabó, N Thomas, S Udry, V Van Grootel, N A Walton

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, ⟨10.1093/mnras/stac2565⟩
Monthly Notices of the Royal Astronomical Society, 519(3), 3546–3563
Sebastian, D; Swayne, M I; Maxted, P F L; Triaud, A H M J; Sousa, S G; Olofsson, G; Beck, M; Billot, N; Hoyer, S; Gill, S; Heidari, N; Martin, D V; Persson, C M; Standing, M R; Alibert, Y; Alonso, R; Anglada, G; Asquier, J; Bárczy, T; Barrado, D; ... (2023). The EBLM project – IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curves. Monthly notices of the Royal Astronomical Society, 519(3), pp. 3546-3563. Oxford University Press 10.1093/mnras/stac2565

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 r

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6527787c8316b9f6242507e4365e810
https://eprints.keele.ac.uk/11469/1/stac2565.pdf