Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Cilia Damiani"'
Autor:
Isabelle Boisse, François Bouchy, G. Bruno, G. Montagnier, Cilia Damiani, Magali Deleuil, S. C. C. Barros, Aldo S. Bonomo, Alexandre Santerne, J. M. Almenara, Guillaume Hébrard, Rodrigo F. Díaz
Publikováno v:
The Space Photometry Revolution-CoRoT Symposium 3
The Space Photometry Revolution-CoRoT Symposium 3, 0000, à renseigner, Unknown Region. p. 471-476., ⟨10.1051/epjconf/201510106014⟩
EPJ Web of Conferences, Vol 101, p 06014 (2015)
The Space Photometry Revolution-CoRoT Symposium 3, 0000, à renseigner, Unknown Region. p. 471-476., ⟨10.1051/epjconf/201510106014⟩
EPJ Web of Conferences, Vol 101, p 06014 (2015)
International audience; We present the analysis of the multi-planetary system Kepler-117, which is part of our program of observations of Kepler planets. This system is composed of a ~ 30 MEarth planet in a ~ 19 days orbit and a ~ 2 MJ planet orbitin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5c4fb0d6f42f6136a97372ce377dfab
https://hal-insu.archives-ouvertes.fr/insu-03581047
https://hal-insu.archives-ouvertes.fr/insu-03581047
Autor:
Damien Fournier, Zhi-Chao Liang, Yuto Bekki, Robert H. Cameron, Bastian Proxauf, Cilia Damiani, Laura Hyest, Aaron C. Birch, B. Lekshmi, Allan Sacha Brun, Laurent Gizon, Richard S. Bogart, Kiran Jain
The oscillations of a slowly rotating star have long been classified into spheroidal and toroidal modes. The spheroidal modes include the well-known 5-min acoustic modes used in helioseismology. Here we report observations of the Sun's toroidal modes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9e91ccc143d0a9b3a3492d3215c80e3
http://arxiv.org/abs/2107.09499
http://arxiv.org/abs/2107.09499
Autor:
D. Rouan, Davide Gandolfi, Aldo S. Bonomo, François Bouchy, S. C. C. Barros, Eike W. Guenther, Anders Erikson, Heike Rauer, O. L. Creevey, M. Pätzold, M. Fridlund, Tsevi Mazeh, Suzanne Aigrain, Jean Schneider, Hans J. Deeg, Günther Wuchterl, A. Baglin, Peter Klagyivik, Sz. Csizmadia, Sascha Grziwa, M. Deleuil, Hannu Parviainen, A. P. Hatzes, Guillaume Hébrard, J. Cabrera, Marc Ollivier, Pascal Bordé, J. M. Almenara, Cilia Damiani, T. Guillot, Alexandre Santerne, Sylvio Ferraz-Mello, Roi Alonso, Rodrigo F. Díaz
Publikováno v:
Astronomy & Astrophysics, 635, A122
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A122. ⟨10.1051/0004-6361/201732393⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A122. ⟨10.1051/0004-6361/201732393⟩
Aims. We report the discovery as well as the orbital and physical characterizations of two new transiting giant exoplanets, CoRoT-30 b and CoRoT-31 b, with the CoRoT space telescope. Methods. We analyzed two complementary data sets: photometric trans
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b600087dcc3b0607a6ec326eb57686b
http://hdl.handle.net/2318/1791021
http://hdl.handle.net/2318/1791021
Publikováno v:
Astronomy & Astrophysics
Large-scale Rossby waves have recently been discovered from measurements of horizontal surface and near-surface solar flows (L\"optien at al. 2018). We are interested in understanding why only the sectoral modes are seen in the observations and also
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb011cf8838339b290b724be1b7cdc25
Autor:
M. Benbakoura, Jean McKeever, Anne Hedlund, Jason Jackiewicz, Drew Chojnowski, Mathieu Vrard, Benoit Mosser, Patrick Gaulme, Cilia Damiani, Federico Spada
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A63. ⟨10.1051/0004-6361/202037781⟩
Astronomy and Astrophysics-A&A, 2020, 639, pp.A63. ⟨10.1051/0004-6361/202037781⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A63. ⟨10.1051/0004-6361/202037781⟩
Astronomy and Astrophysics-A&A, 2020, 639, pp.A63. ⟨10.1051/0004-6361/202037781⟩
The objective of this work is to determine what fraction of red-giant (RG) stars shows photometric rotational modulation, and understand its origin. One of the underlying questions is the role of close binarity in this population, standing upon the f
Autor:
S. C. C. Barros, Isabelle Boisse, B. Courcol, Aldo S. Bonomo, Paul Wilson, Alexandre Santerne, Guillaume Hébrard, J. M. Almenara, Magali Deleuil, Rodrigo F. Díaz, Xavier Bonfils, Stéphane Udry, François Bouchy, Cilia Damiani, Olivier Demangeon, Rosemary A. Mardling, J. Rey
Publikováno v:
Astronomy and Astrophysics, 615, A90
Astronomy and Astrophysics
Astronomy and Astrophysics, EDP Sciences, 2018, 615, pp.A90. ⟨10.1051/0004-6361/201732500⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 615, pp.A90. ⟨10.1051/0004-6361/201732500⟩
Astronomy and Astrophysics
Astronomy and Astrophysics, EDP Sciences, 2018, 615, pp.A90. ⟨10.1051/0004-6361/201732500⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 615, pp.A90. ⟨10.1051/0004-6361/201732500⟩
Kepler-419 is a planetary system discovered by the Kepler photometry which is known to harbour two massive giant planets: [...] Here we present new radial velocity (RV) measurements secured over more than two years with the SOPHIE spectrograph, where
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::29c3b2ab5497ee651d7f7f98536d8375
Autor:
Cilia Damiani, Stéphane Mathis
Publikováno v:
Astronomy & Astrophysics
It is debated whether close-in giant planets can form in-situ and if not, which mechanisms are responsible for their migration. One of the observable tests for migration theories is the current value of the angle between the stellar equatorial plane
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe647112859fa32982996dbf1cd9f67f
Autor:
A. Lecavelier des Etangs, Andre Izidoro, Artie P. Hatzes, Suzanne Aigrain, Davide Gandolfi, Juan Cabrera, Sz. Csizmadia, Heike Rauer, Guillaume Hébrard, Pascal Borde, Daniel Rouan, François Bouchy, Marc Ollivier, C. Moutou, Martin Pätzold, E. W. Guenther, Alexandre Santerne, Hans J. Deeg, Malcolm Fridlund, Roi Alonso, C. Lovis, Rodrigo F. Díaz, Anders Erikson, Tristan Guillot, Magali Deleuil, Jose-Manuel Almenara, Sean N. Raymond, Cilia Damiani, Aldo S. Bonomo, J. Schneider
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 603, pp.id.A43. ⟨10.1051/0004-6361/201730624⟩
Astronomy & Astrophysics (0004-6361), 603, A43
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A, 2017, 603, pp.id.A43. ⟨10.1051/0004-6361/201730624⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 603, pp.id.A43. ⟨10.1051/0004-6361/201730624⟩
Astronomy & Astrophysics (0004-6361), 603, A43
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A, 2017, 603, pp.id.A43. ⟨10.1051/0004-6361/201730624⟩
CoRoT-9b is one of the rare long-period (P=95.3 days) transiting giant planets with a measured mass known to date. We present a new analysis of the CoRoT-9 system based on five years of radial-velocity (RV) monitoring with HARPS and three new space-b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cdb2b80d7854837dbaaaac594bf6ee3f
https://hal.archives-ouvertes.fr/hal-01493751
https://hal.archives-ouvertes.fr/hal-01493751
Autor:
Rodrigo F. Díaz, Cilia Damiani
Brown dwarfs straddle the mass range transition from planetary to stellar objects. There is a relative paucity of brown dwarfs companions around FGKM stars compared to exoplanets for orbital periods less than a few years, but most of the short-period
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e4fcc0600ec39bd304a384e2f87c988
http://arxiv.org/abs/1602.07098
http://arxiv.org/abs/1602.07098
Autor:
Rodrigo F. Díaz, Cilia Damiani, J. M. Almenara, Rosemary A. Mardling, Magali Deleuil, X. Bonfils, G. Bruno, S. C. C. Barros
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, 2015, 453 (3), pp.2644--2652. ⟨10.1093/mnras/stv1735⟩
Monthly Notices of the Royal Astronomical Society, 2015, 453 (3), pp.2644--2652. ⟨10.1093/mnras/stv1735⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 453 (3), pp.2644--2652. ⟨10.1093/mnras/stv1735⟩
Monthly Notices of the Royal Astronomical Society, 2015, 453 (3), pp.2644--2652. ⟨10.1093/mnras/stv1735⟩
The masses and radii of extrasolar planets are key observables for understanding their interior, formation and evolution. While transit photometry and Doppler spectroscopy are used to measure the radii and masses respectively of planets relative to t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4fe85f34aa0d4d83872bcf25216a897
https://hal.archives-ouvertes.fr/hal-01439824
https://hal.archives-ouvertes.fr/hal-01439824