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

Optical and near-infrared stellar activity characterization of the early M dwarf Gl 205 with SOPHIE and SPIRou

Autor: P. Cortés-Zuleta, I. Boisse, B. Klein, E. Martioli, P. I. Cristofari, A. Antoniadis-Karnavas, J.-F. Donati, X. Delfosse, C. Cadieux, N. Heidari, É. Artigau, S. Bellotti, X. Bonfils, A. Carmona, N. J. Cook, R. F. Díaz, R. Doyon, P. Fouqué, C. Moutou, P. Petit, T. Vandal, L. Acuña, L. Arnold, N. Astudillo-Defru, V. Bourrier, F. Bouchy, R. Cloutier, S. Dalal, M. Deleuil, O. D. S. Demangeon, X. Dumusque, T. Forveille, J. Gomes da Silva, N. Hara, G. Hébrard, S. Hoyer, G. Hussain, F. Kiefer, J. Morin, A. Santerne, N. C. Santos, D. Segransan, M. Stalport, S. Udry

Publikováno v: Astronomy & Astrophysics. 673:A14

The stellar activity of M dwarfs is the main limitation for discovering and characterizing exoplanets orbiting them since it induces quasi-periodic RV variations. We aim to characterize the magnetic field and stellar activity of the early, moderately

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https://doi.org/10.1051/0004-6361/202245131

Characterization of the HD 108236 system with CHEOPS and TESS Confirmation of a fifth transiting planet

Autor: S. Hoyer, A. Bonfanti, A. Leleu, L. Acuña, L. M. Serrano, M. Deleuil, A. Bekkelien, C. Broeg, H.-G. Florén, D. Queloz, T. G. Wilson, S. G. Sousa, M. J. Hooton, V. Adibekyan, Y. Alibert, R. Alonso, G. Anglada, J. Asquier, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, M. Beck, T. Beck, W. Benz, N. Billot, F. Biondi, X. Bonfils, A. Brandeker, J. Cabrera, S. Charnoz, A. Collier Cameron, Sz. Csizmadia, M. B. Davies, L. Delrez, O. D. S. Demangeon, B.-O. Demory, D. Ehrenreich, A. Erikson, A. Fortier, L. Fossati, M. Fridlund, D. Gandolfi, M. Gillon, M. Güdel, N. Hara, K. Heng, K. G. Isaak, J. M. Jenkins, L. L. Kiss, J. Laskar, D. W. Latham, A. Lecavelier des Etangs, M. Lendl, C. Lovis, A. Luntzer, D. Magrin, P. F. L. Maxted, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, E. Pallé, C. M. Persson, G. Peter, D. Piazza, G. Piotto, D. Pollacco, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, G. R. Ricker, S. Salmon, N. C. Santos, G. Scandariato, S. Seager, D. Ségransan, A. E. Simon, A. M. S. Smith, M. Steller, Gy. M. Szabó, N. Thomas, J. D. Twicken, S. Udry, V. Van Grootel, R. K. Vanderspek, N. A. Walton, K. Westerdorff, J. N. Winn

Publikováno v: Astronomy & Astrophysics, 668:A117
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 668, ⟨10.1051/0004-6361/202243720⟩
Hoyer, S.; Bonfanti, A.; Leleu, A.; Acuña, L.; Serrano, L. M.; Deleuil, M.; Bekkelien, A.; Broeg, C.; Florén, H.-G.; Queloz, D.; Wilson, T. G.; Sousa, S. G.; Hooton, M. J.; Adibekyan, V.; Alibert, Y.; Alonso, R.; Anglada, G.; Asquier, J.; Bárczy, T.; Barrado, D.; ... (2022). Characterization of the HD 108236 system with CHEOPS and TESS Confirmation of a fifth transiting planet. Astronomy and astrophysics, 668, A117. EDP Sciences 10.1051/0004-6361/202243720

S. Hoyer et al.
[Context] The HD 108236 system was first announced with the detection of four small planets based on TESS data. Shortly after, the transit of an additional planet with a period of 29.54 d was serendipitously detected by CHEOPS. I

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https://refubium.fu-berlin.de/handle/fub188/38331

$\tt{KOBEsim}$: a Bayesian observing strategy algorithm for planet detection in radial velocity blind-search surveys

Autor: O. Balsalobre-Ruza, J. Lillo-Box, A. Berihuete, A. M. Silva, N. C. Santos, A. Castro-González, J. P. Faria, N. Huélamo, D. Barrado, O. D. S. Demangeon, E. Marfil, J. Aceituno, V. Adibekyan, M. Azzaro, S. C. C. Barros, G. Bergond, D. Galadí-Enríquez, S. Pedraz, A. Santerne

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2023, 669, ⟨10.1051/0004-6361/202243938⟩

This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid

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The young HD 73583 (TOI-560) planetary system: Two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf

Autor: O Barragán, D J Armstrong, D Gandolfi, I Carleo, A A Vidotto, C Villarreal D’Angelo, A Oklopčić, H Isaacson, D Oddo, K Collins, M Fridlund, S G Sousa, C M Persson, C Hellier, S Howell, A Howard, S Redfield, N Eisner, I Y Georgieva, D Dragomir, D Bayliss, L D Nielsen, B Klein, S Aigrain, M Zhang, J Teske, J D Twicken, J Jenkins, M Esposito, V Van Eylen, F Rodler, V Adibekyan, J Alarcon, D R Anderson, J M Akana Murphy, D Barrado, S C C Barros, B Benneke, F Bouchy, E M Bryant, R P Butler, J Burt, J Cabrera, S Casewell, P Chaturvedi, R Cloutier, W D Cochran, J Crane, I Crossfield, N Crouzet, K I Collins, F Dai, H J Deeg, A Deline, O D S Demangeon, X Dumusque, P Figueira, E Furlan, C Gnilka, M R Goad, E Goffo, F Gutiérrez-Canales, A Hadjigeorghiou, Z Hartman, A P Hatzes, M Harris, B Henderson, T Hirano, S Hojjatpanah, S Hoyer, P Kabáth, J Korth, J Lillo-Box, R Luque, M Marmier, T Močnik, A Muresan, F Murgas, E Nagel, H L M Osborne, A Osborn, H P Osborn, E Palle, M Raimbault, G R Ricker, R A Rubenzahl, C Stockdale, N C Santos, N Scott, R P Schwarz, S Shectman, S Seager, D Ségransan, L M Serrano, M Skarka, A M S Smith, J Šubjak, T G Tan, S Udry, C Watson, P J Wheatley, R West, J N Winn, S X Wang, A Wolfgang, C Ziegler

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, ⟨10.1093/mnras/stac638⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 514(2), 1606-1627. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 514(2), 1606-1627
Barragán, O, Armstrong, D J, Gandolfi, D, Carleo, I, Vidotto, A A, Villarreal D’Angelo, C, Oklopčić, A, Isaacson, H, Oddo, D, Collins, K I, Fridlund, M, Sousa, S G, Persson, C M, Hellier, C, Howell, S, Howard, A, Redfield, S, Eisner, N, Georgieva, I Y, Dragomir, D, Bayliss, D, Nielsen, L D, Klein, B, Aigrain, S, Zhang, M, Teske, J, Twicken, J D, Jenkins, J, Esposito, M, Van Eylen, V, Rodler, F, Adibekyan, V, Alarcon, J, Anderson, D R, Akana Murphy, J M, Barrado, D, Barros, S C C, Benneke, B, Bouchy, F, Bryant, E M, Butler, R P, Burt, J, Cabrera, J, Casewell, S, Chaturvedi, P, Cloutier, R, Cochran, W D, Crane, J, Crossfield, I, Crouzet, N, Collins, K I, Dai, F, Deeg, H J, Deline, A, Demangeon, O D S, Dumusque, X, Figueira, P, Furlan, E, Gnilka, C, Goad, M R, Goffo, E, Gutiérrez-Canales, F, Hadjigeorghiou, A, Hartman, Z, Hatzes, A P, Harris, M, Henderson, B, Hirano, T, Hojjatpanah, S, Hoyer, S, Kabáth, P, Korth, J, Lillo-Box, J, Luque, R, Marmier, M, Močnik, T, Muresan, A, Murgas, F, Nagel, E, Osborne, H L M, Osborn, A, Osborn, H P, Palle, E, Raimbault, M, Ricker, G R, Rubenzahl, R A, Stockdale, C, Santos, N C, Scott, N, Schwarz, R P, Shectman, S, Raimbault, M, Seager, S, Ségransan, D, Serrano, L M, Skarka, M, Smith, A M S, Šubjak, J, Tan, T G, Udry, S, Watson, C, Wheatley, P J, West, R, Winn, J N, Wang, S X, Wolfgang, A & Ziegler, C 2022, ' The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 2, pp. 1606-1627 . https://doi.org/10.1093/mnras/stac638

This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origina

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https://hal-insu.archives-ouvertes.fr/insu-03667449/document