Zobrazeno 1 - 10
of 53
pro vyhledávání: '"B. Toledo-Padrón"'
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
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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:
J. Maldonado, A. Petralia, M. Damasso, M. Pinamonti, G. Scandariato, E. González-Álvarez, L. Affer, G. Micela, A. F. Lanza, G. Leto, E. Poretti, A. Sozzetti, M. Perger, P. Giacobbe, R. Zanmar Sánchez, A. Maggio, J. I. González Hernández, R. Rebolo, I. Ribas, A. Suárez-Mascareño, B. Toledo-Padrón, A. Bignamini, E. Molinari, E. Covino, R. Claudi, S. Desidera, E. Herrero, J. C. Morales, I. Pagano, G. Piotto
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
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DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
[Context] It is now well-established that small, rocky planets are common around low-mass stars. However, the detection of such planets is challenged by the short-term activity of host stars. [Aims] The HARPS-N red Dwarf Exoplanet Survey programme is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ea2df49d489cf0491a8aad9b24c109f
http://hdl.handle.net/10261/257811
http://hdl.handle.net/10261/257811
Autor:
Carlos González-Fernández, Sergio Simón-Díaz, Emilio Molinari, Thomas Masseron, G. Holgado, Tabetha S. Boyajian, Jason T. Wright, A. Collier Cameron, Grant M. Kennedy, J. Saario, Hector Socas-Navarro, M. J. Martínez González, B. Toledo-Padrón, J. I. González Hernández, A. Asensio Ramos, C. Westendorp Plaza
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 486:236-244
Boyajian's star is an apparently normal main sequence F-type star with a very unusual light curve. The dipping activity of the star, discovered during the Kepler mission, presents deep, asymmetric, and aperiodic events. Here we present high resolutio
Autor:
J. I. González Hernández, Matteo Pinamonti, M. Perger, R. Zanmar Sanchez, Antonio Maggio, Isabella Pagano, E. González-Álvarez, Andrea Bignamini, Jorge Maldonado, Rafael Rebolo, Alessandro Sozzetti, Giuseppina Micela, Giuseppe Leto, L. Affer, Paolo Giacobbe, B. Toledo-Padrón, Ennio Poretti, A. Petralia, Ignasi Ribas, Elvira Covino, Antonino F. Lanza, A. Suárez Mascareño, Mario Damasso, Gaetano Scandariato
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
[Context] The high number of super-Earth and Earth-like planets in the habitable zone detected around M-dwarf stars in recent years has revealed these stellar objects to be the key to planetary radial velocity (RV) searches. [Aims] Using the HARPS-N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27eba3a275b19135565b25c487488fb1
http://hdl.handle.net/10261/257744
http://hdl.handle.net/10261/257744
Autor:
Tobias Wilken, J. I. González Hernández, Matthias Steffen, A. Suárez Mascareño, Ronald Holzwarth, B. Toledo-Padrón, Hans-Günter Ludwig, Elisabetta Caffau, Paolo Molaro, Massimiliano Esposito, L. Pasquini, Tilo Steinmetz, G. Lo Curto, Rafael Rebolo, Theodor W. Hänsch, Antonio Manescau, Rafael A. Probst, Thomas Udem
Publikováno v:
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A146. ⟨10.1051/0004-6361/202038937⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A146. ⟨10.1051/0004-6361/202038937⟩
The General Theory of Relativity predicts the redshift of spectral lines in the solar photosphere, as a consequence of the gravitational potential of the Sun. This effect can be measured from a solar disk-integrated flux spectrum of the Sun's reflect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e079db32e3496ab0fcf422695c3707d
https://hdl.handle.net/21.11116/0000-0008-9647-F21.11116/0000-0008-9645-1
https://hdl.handle.net/21.11116/0000-0008-9647-F21.11116/0000-0008-9645-1
Autor:
Dinko Milaković, Ronald Holzwarth, Thomas Udem, B. Toledo-Padrón, Antonio Manescau, Jonay I. González Hernández, Massimiliano Esposito, Yuanjie Wu, Frank Grupp, Anna Brucalassi, Josefina Urrutia, Hanna Kellermann, Luca Pasquini, Bruno L. Canto Martins, Florian Kerber, Alejandro Suárez Mascareño, Rafael Rebolo, Rafael A. Probst, Gaspare Lo Curto, Theodor W. Hänsch, I. C. Leão, José Renan de Medeiros, Eszter Pozna, Olaf Mandel, Tilo Steinmetz, Gerardo Avila
Publikováno v:
Nature astronomy
Laser frequency combs (LFCs) are well on their way to becoming the next-generation calibration sources for precision astronomical spectroscopy. This development is considered key in the hunt for low-mass rocky exoplanets around solar-type stars whose
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62c28bc3d33b014de20cb397622384b5
http://arxiv.org/abs/2002.08868
http://arxiv.org/abs/2002.08868
Autor:
Claudio Cumani, João Coelho, Luca Oggioni, Nelson J. Nunes, Alessio Zanutta, Matteo Genoni, Antonio Manescau, Jorge Lillo-Box, François Bouchy, A. Segovia, Nuno C. Santos, M. Moschetti, M. Affolter, L. Genolet, A. Fragoso, Paolo Spanò, G. Lo Curto, Pedro Figueira, Valentina D'Odorico, Alessandro Sozzetti, C. Broeg, Alexandre Cabral, Andrea Mehner, J. L. Rasilla, Marco Riva, B. Toledo-Padrón, Roberto Cirami, I. Hughes, C. Lovis, Rafael Rebolo, Hugo M. Tabernero, Francesco Pepe, L. Pasquini, Willy Benz, Ennio Poretti, Marco Landoni, B. Lavie, T. Bandy, Yann Alibert, Antonio Cesar de Oliveira, Diego Bossini, A. Suárez Mascareño, Mahmoudreza Oshagh, C. Allende Prieto, Stefano Cristiani, Filippo Maria Zerbi, M. A. Monteiro, S. Deiries, Danuta Sosnowska, Carlos Martins, Paolo Conconi, R. Génova Santos, F. Tenegi, Charles Maire, Igor Coretti, Matteo Aliverti, S. C. C. Barros, E. Mueller, J. I. González Hernández, Andrea Modigliani, Serena Benatti, B. Delabre, David Alves, M. Amate, Olaf Iwert, V. Baldini, Stéphane Udry, G. Cupani, Hans Dekker, P. Di Marcantonio, Pedro Santos, V. Adibekyan, Giorgio Calderone, D. Mégevand, M. R. Zapatero Osorio, Manuel Abreu, S. Santana Tschudi, J. Knudstrup, Romain Allart, Andrea Bianco, Olivier Demangeon, Paolo Molaro, Paolo Santin, Mario Damasso, Enric Palle, S. G. Sousa, Giorgio Pariani, J.-L. Lizon, Gerardo Avila, David Ehrenreich, Edoardo Maria Alberto Redaelli, Mário J. P. F. G. Monteiro, Giuseppina Micela
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
Toledo-Padrón, B. et al.
Context. An accurate characterization of the known exoplanet population is key to understanding the origin and evolution of planetary systems. Determining true planetary masses through the radial velocity (RV) method is
Context. An accurate characterization of the known exoplanet population is key to understanding the origin and evolution of planetary systems. Determining true planetary masses through the radial velocity (RV) method is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::630a8a923cb37896d5e7b98b4b0faaaa
http://hdl.handle.net/10261/233763
http://hdl.handle.net/10261/233763
Autor:
Andrea Bignamini, Daniele Locci, Katia Biazzo, Ennio Poretti, Riccardo Claudi, Giuseppina Micela, Enrique Herrero, C. Di Maio, Ignasi Ribas, Rafael Rebolo, A. Suárez-Mascareño, G. Piotto, Alessandro Sozzetti, Elvira Covino, Juan Carlos Morales, B. Toledo-Padrón, A. Petralia, Antonino F. Lanza, Valentina D'Orazi, J. I. González Hernández, M. Baratella, Silvano Desidera, Emilio Molinari, Gaetano Scandariato, L. Affer, Matteo Pinamonti, Isabella Pagano, Antonio Maggio, M. Perger, Jesus Maldonado
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
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[Context] Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing.
[Aims] Correlati
[Aims] Correlati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0a1b270ddf2a6f9320c8e701fa133bb
http://hdl.handle.net/10261/232773
http://hdl.handle.net/10261/232773
Autor:
E. González-Álvarez, Ignasi Ribas, Alessandro Sozzetti, M. Perger, B. Toledo-Padrón, Mario Damasso, Ansgar Reiners, Paolo Giacobbe, J. A. Caballero, Rafael Rebolo, A. Suárez Mascareño, Giuseppe Leto, Enrique Herrero, L. Affer, R. Zanmar Sanchez, Giuseppina Micela, Mathias Zechmeister, J. I. González Hernández, Isabella Pagano, Juan Carlos Morales, Matteo Pinamonti, Gaetano Scandariato, P. J. Amado, Jesus Maldonado, Silvano Desidera, Andreas Quirrenbach
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Context. M-dwarfs have proven to be ideal targets for planetary radial velocity (RV) searches due to their higher planet-star mass contrast, which favors the detection of low-mass planets. The abundance of super-Earth and Earth-like planets detected
Autor:
D S Aguado, C. González Gutiérrez, E. Díez Alonso, Laura Bonavera, A. Suárez Mascareño, Sergio Luis Suárez Gómez, B. Toledo-Padrón, J. Carballido-Landeira, J. I. González Hernández, Rafael Rebolo, Antonio Cabrera-Lavers, F. J. de Cos Juez
Publikováno v:
WOS:000489302400105
RUO. Repositorio Institucional de la Universidad de Oviedo
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RUO. Repositorio Institucional de la Universidad de Oviedo
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We present a super-Earth orbiting close to the inner edge of the habitable zone of the cool dwarf star K2-286 (EPIC 249889081), detected with data from the K2 mission in its $15^{th}$ campaign. The planet has radius of $2.1\pm0.2$ R$_{\oplus}$, near
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1de8493b30ef37b7037dcbd8e6aa9fd6
http://hdl.handle.net/10651/53732
http://hdl.handle.net/10651/53732