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of 394
pro vyhledávání: '"F. Marzari"'
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
Akademický článek
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Autor:
M. Damasso, D. Locci, S. Benatti, A. Maggio, D. Nardiello, M. Baratella, K. Biazzo, A. S. Bonomo, S. Desidera, V. D'Orazi, M. Mallonn, A. F. Lanza, A. Sozzetti, F. Marzari, F. Borsa, J. Maldonado, L. Mancini, E. Poretti, G. Scandariato, A. Bignamini, L. Borsato, R. Capuzzo Dolcetta, M. Cecconi, R. Claudi, R. Cosentino, E. Covino, A. Fiorenzano, A. Harutyunyan, A. W. Mann, G. Micela, E. Molinari, M. Molinaro, I. Pagano, M. Pedani, M. Pinamonti, G. Piotto, H. Stoev
For more than two years, we monitored with the HARPS-N spectrograph the 400 Myr-old star HD\,63433, which hosts two close-in (orbital periods $P_b\sim7.1$ and $P_c\sim20.5$ days) sub-Neptunes detected by the TESS space telescope, and it was announced
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64044c8aaca620414ba7fe83c67d12ba
https://hdl.handle.net/2108/327643
https://hdl.handle.net/2108/327643
Autor:
A. Suárez Mascareño, M. Damasso, N. Lodieu, A. Sozzetti, V. J. S. Béjar, S. Benatti, M. R. Zapatero Osorio, G. Micela, R. Rebolo, S. Desidera, F. Murgas, R. Claudi, J. I. González Hernández, L. Malavolta, C. del Burgo, V. D’Orazi, P. J. Amado, D. Locci, H. M. Tabernero, F. Marzari, D. S. Aguado, D. Turrini, C. Cardona Guillén, B. Toledo-Padrón, A. Maggio, J. Aceituno, F. F. Bauer, J. A. Caballero, P. Chinchilla, E. Esparza-Borges, E. González-Álvarez, T. Granzer, R. Luque, E. L. Martín, G. Nowak, M. Oshagh, E. Pallé, H. Parviainen, A. Quirrenbach, A. Reiners, I. Ribas, K. G. Strassmeier, M. Weber, M. Mallonn
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years1,2. These theoretical expectations remai
Autor:
A. Zurlo, K. Goździewski, C. Lazzoni, D. Mesa, P. Nogueira, S. Desidera, R. Gratton, F. Marzari, M. Langlois, E. Pinna, G. Chauvin, P. Delorme, J. H. Girard, J. Hagelberg, Th. Henning, M. Janson, E. Rickman, P. Kervella, H. Avenhaus, T. Bhowmik, B. Biller, A. Boccaletti, M. Bonaglia, M. Bonavita, M. Bonnefoy, F. Cantalloube, A. Cheetham, R. Claudi, V. D’Orazi, M. Feldt, R. Galicher, E. Ghose, A.-M. Lagrange, H. le Coroller, R. Ligi, M. Kasper, A.-L. Maire, F. Medard, M. Meyer, S. Peretti, C. Perrot, A. T. Puglisi, F. Rossi, B. Rothberg, T. Schmidt, E. Sissa, A. Vigan, Z. Wahhaj
Publikováno v:
Astronomy & Astrophysics, 666
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 666, ⟨10.1051/0004-6361/202243862⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 666, ⟨10.1051/0004-6361/202243862⟩
Context. HR 8799 is a young planetary system composed of four planets and a double debris belt. Being the first multi-planetary system discovered with the direct imaging technique, it has been observed extensively since 1998. This wide baseline of as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1586acd93a4e9319a6779f97a5bc00a3
https://hdl.handle.net/20.500.11850/580555
https://hdl.handle.net/20.500.11850/580555
Akademický článek
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Akademický článek
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Autor:
K. Biazzo, V. D’Orazi, S. Desidera, D. Turrini, S. Benatti, R. Gratton, L. Magrini, A. Sozzetti, M. Baratella, A. S. Bonomo, F. Borsa, R. Claudi, E. Covino, M. Damasso, M. P. Di Mauro, A. F. Lanza, A. Maggio, L. Malavolta, J. Maldonado, F. Marzari, G. Micela, E. Poretti, F. Vitello, L. Affer, A. Bignamini, I. Carleo, R. Cosentino, A. F. M. Fiorenzano, P. Giacobbe, A. Harutyunyan, G. Leto, L. Mancini, E. Molinari, M. Molinaro, D. Nardiello, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, M. Rainer, G. Scandariato
Context. Exoplanetary properties strongly depend on stellar properties: to know the planet with accuracy and precision it is necessary to know the star as accurately and precisely as possible. Aims. Our immediate aim is to characterize in a homogeneo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39a9212cc5d693cdd5f98c525632f359
https://hdl.handle.net/11577/3454816
https://hdl.handle.net/11577/3454816
Autor:
M. Steller, Magali Deleuil, Roberto Ragazzoni, G. Scandariato, Nascimbeni, J. Asquier, László L. Kiss, Yann Alibert, C. Broeg, Nuno C. Santos, David Barrado, Enric Palle, Damien Ségransan, Andrea Fortier, Don Pollacco, Monika Lendl, B.-O. Demory, T. G. Wilson, Demetrio Magrin, Giampaolo Piotto, Nicola Rando, T. Bandy, M. Fridlund, J. Hasiba, Michaël Gillon, Van Grootel, J. Cabrera, David Ehrenreich, Anders Erikson, Alexis Brandeker, Willy Benz, K. G. Isaak, N. A. Walton, I. Pagano, Jacques Laskar, E. Kopp, G. Escude, G. Olofsson, Z. Garai, Olivier Demangeon, C. Lovis, Pierre F. L. Maxted, Wolfgang Baumjohann, S. C. C. Barros, Nicolas Billot, Kevin Heng, Manuel Guedel, Sébastien Charnoz, Thomas Beck, T. Bárczy, Xavier Bonfils, Gyula M. Szabó, Szilard Csizmadia, A L des Etangs, Alexis M. S. Smith, Matteo Munari, L. Delrez, A. E. Simon, G. Lacedelli, L. Borsato, Sérgio F. Sousa, Didier Queloz, F. Marzari, Davide Gandolfi, L M Serrano, N. Thomas, Andrew Collier Cameron, Roi Alonso, Ignasi Ribas, Stéphane Udry, M. Beck, Sergio Hoyer, A. Bonfanti, Melvyn B. Davies, Heike Rauer, Luca Fossati, Gisbert Peter, Roland Ottensamer
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 506 (3), pp.3810-3830. ⟨10.1093/mnras/stab1782⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Borsato, L; Piotto, G; Gandolfi, D; Nascimbeni, V; Lacedelli, G; Marzari, F; Billot, N; Maxted, P F L; Sousa, S; Cameron, A C; Bonfanti, A; Wilson, T G; Serrano, L M; Garai, Z; Alibert, Y; Alonso, R; Asquier, J; Bárczy, T; Bandy, T; Barrado, D; ... (2021). Exploiting timing capabilities of the CHEOPS mission with warm-Jupiter planets. Monthly notices of the Royal Astronomical Society, 506(3), pp. 3810-3830. Oxford University Press 10.1093/mnras/stab1782
Monthly Notices of the Royal Astronomical Society, 506(3), 3810-3830
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 506 (3), pp.3810-3830. ⟨10.1093/mnras/stab1782⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Borsato, L; Piotto, G; Gandolfi, D; Nascimbeni, V; Lacedelli, G; Marzari, F; Billot, N; Maxted, P F L; Sousa, S; Cameron, A C; Bonfanti, A; Wilson, T G; Serrano, L M; Garai, Z; Alibert, Y; Alonso, R; Asquier, J; Bárczy, T; Bandy, T; Barrado, D; ... (2021). Exploiting timing capabilities of the CHEOPS mission with warm-Jupiter planets. Monthly notices of the Royal Astronomical Society, 506(3), pp. 3810-3830. Oxford University Press 10.1093/mnras/stab1782
Monthly Notices of the Royal Astronomical Society, 506(3), 3810-3830
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a396354810359c7fa673a40ce6f82e2c
https://hal-insu.archives-ouvertes.fr/insu-03458350
https://hal-insu.archives-ouvertes.fr/insu-03458350