Zobrazeno 1 - 10
of 59
pro vyhledávání: '"V J S Béjar"'
Context. Open clusters (OCs) are fundamental benchmarks where theories of star formation and stellar evolution can be tested and validated. Coma Ber and Latyshev 2 (Group X) are the second and third OCs closest to the Sun, making them excellent targe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7fbe86d043b23f925f1a596e417baa63
http://arxiv.org/abs/2304.08618
http://arxiv.org/abs/2304.08618
Autor:
M. Mallorquín, V. J. S. Béjar, N. Lodieu, M. R. Zapatero Osorio, H. Tabernero, A. Suárez Mascareño, M. Zechmeister, R. Luque, E. Pallé, D. Montes
Context. Although the number of exoplanets reported in the literature exceeds 5000 so far, only a few dozen of them are young planets (≤900 Myr). However, a complete characterization of these young planets is key to understanding the current proper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be399163920c213ae119cd0bf57b396f
http://arxiv.org/abs/2303.15411
http://arxiv.org/abs/2303.15411
Autor:
I. Ribas, A. Reiners, M. Zechmeister, J. A. Caballero, J. C. Morales, S. Sabotta, D. Baroch, P. J. Amado, A. Quirrenbach, M. Abril, J. Aceituno, G. Anglada-Escudé, M. Azzaro, D. Barrado, V. J. S. Béjar, D. Benítez de Haro, G. Bergond, P. Bluhm, R. Calvo Ortega, C. Cardona Guillén, P. Chaturvedi, C. Cifuentes, J. Colomé, D. Cont, M. Cortés-Contreras, S. Czesla, E. Díez-Alonso, S. Dreizler, C. Duque-Arribas, N. Espinoza, M. Fernández, B. Fuhrmeister, D. Galadí-Enríquez, A. García-López, E. González-Álvarez, J. I. González Hernández, E. W. Guenther, E. de Guindos, A. P. Hatzes, Th. Henning, E. Herrero, D. Hintz, Á. L. Huelmo, S. V. Jeffers, E. N. Johnson, E. de Juan, A. Kaminski, J. Kemmer, J. Khaimova, S. Khalafinejad, D. Kossakowski, M. Kürster, F. Labarga, M. Lafarga, S. Lalitha, M. Lampón, J. Lillo-Box, N. Lodieu, M. J. López González, M. López-Puertas, R. Luque, H. Magán, L. Mancini, E. Marfil, E. L. Martín, S. Martín-Ruiz, K. Molaverdikhani, D. Montes, E. Nagel, L. Nortmann, G. Nowak, E. Pallé, V. M. Passegger, A. Pavlov, S. Pedraz, V. Perdelwitz, M. Perger, A. Ramón-Ballesta, S. Reffert, D. Revilla, E. Rodríguez, C. Rodríguez-López, S. Sadegi, M. Á. Sánchez Carrasco, A. Sánchez-López, J. Sanz-Forcada, S. Schäfer, M. Schlecker, J. H. M. M. Schmitt, P. Schöfer, A. Schweitzer, W. Seifert, Y. Shan, S. L. Skrzypinski, E. Solano, O. Stahl, M. Stangret, S. Stock, J. Stürmer, H. M. Tabernero, L. Tal-Or, T. Trifonov, S. Vanaverbeke, F. Yan, M. R. Zapatero Osorio
Publikováno v:
Astronomy and Astrophysics
The CARMENES instrument was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The broad wavelength coverage was designed to provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b8cfde360b03faee5da32e1d3b118d3
https://hdl.handle.net/21.11116/0000-000C-B462-A
https://hdl.handle.net/21.11116/0000-000C-B462-A
Autor:
J. Blanco-Pozo, M. Perger, M. Damasso, G. Anglada Escudé, I. Ribas, D. Baroch, J. A. Caballero, C. Cifuentes, S. V. Jeffers, M. Lafarga, A. Kaminski, S. Kaur, E. Nagel, V. Perdelwitz, M. Pérez-Torres, A. Sozzetti, D. Viganò, P. J. Amado, G. Andreuzzi, V. J. S. Béjar, E. L. Brown, F. Del Sordo, S. Dreizler, D. Galadí-Enríquez, A. P. Hatzes, M. Kürster, A. F. Lanza, A. Melis, E. Molinari, D. Montes, M. Murgia, E. Pallé, L. Peña-Moñino, D. Perrodin, M. Pilia, E. Poretti, A. Quirrenbach, A. Reiners, A. Schweitzer, M. R. Zapatero Osorio, M. Zechmeister
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf77027919a5f79d8528d286d3a46de1
Autor:
J. Šubjak, N. Lodieu, P. Kabáth, H. M. J. Boffin, G. Nowak, F. Grundahl, V. J. S. Béjar, M. R. Zapatero Osorio, V. Antoci
Publikováno v:
Šubjak, J, Lodieu, N, Kabáth, P, Boffin, H M J, Nowak, G, Grundahl, F, Béjar, V J S, Zapatero Osorio, M R & Antoci, V 2023, ' Search for planets around stars with wide brown dwarfs ', Astronomy and Astrophysics, vol. 671, A10 . https://doi.org/10.1051/0004-6361/202244238
Aims. The project aims to understand better the role of wide brown dwarf companions on planetary systems. Methods. We obtained high-resolution spectra of six bright stars with co-moving wide substellar companions with the SONG, CARMENES, and STELLA h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76e1f5d17213feea39a28c61b6a1896d
https://orbit.dtu.dk/en/publications/72356a31-5f0a-42ae-a860-7ae291934bac
https://orbit.dtu.dk/en/publications/72356a31-5f0a-42ae-a860-7ae291934bac
Autor:
D. Kossakowski, M. Kürster, T. Trifonov, Th. Henning, J. Kemmer, J. A. Caballero, R. Burn, S. Sabotta, J. S. Crouse, T. J. Fauchez, E. Nagel, A. Kaminski, E. Herrero, E. Rodríguez, E. González-Álvarez, A. Quirrenbach, P. J. Amado, I. Ribas, A. Reiners, J. Aceituno, V. J. S. Béjar, D. Baroch, S. T. Bastelberger, P. Chaturvedi, C. Cifuentes, S. Dreizler, S. V. Jeffers, R. Kopparapu, M. Lafarga, M. J. López-González, S. Martín-Ruiz, D. Montes, J. C. Morales, E. Pallé, A. Pavlov, S. Pedraz, V. Perdelwitz, M. Pérez-Torres, M. Perger, S. Reffert, C. Rodríguez López, M. Schlecker, P. Schöfer, A. Schweitzer, Y. Shan, A. Shields, S. Stock, E. Wolf, M. R. Zapatero Osorio, M. Zechmeister
Publikováno v:
Astronomy and Astrophysics
We present the discovery of an Earth-mass planet ($M_b\sin i = 1.26\pm0.21M_\oplus$) on a 15.6d orbit of a relatively nearby ($d\sim$9.6pc) and low-mass ($0.167\pm0.011 M_\odot$) M5.0V star, Wolf 1069. Sitting at a separation of $0.0672\pm0.0014$au a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d0f6c669db9fb87600abf790cc0e855
https://hdl.handle.net/21.11116/0000-000C-AB8F-3
https://hdl.handle.net/21.11116/0000-000C-AB8F-3
Autor:
A. Bello-García, V. M. Passegger, J. Ordieres-Meré, A. Schweitzer, J. A. Caballero, A. González-Marcos, I. Ribas, A. Reiners, A. Quirrenbach, P. J. Amado, V. J. S. Béjar, C. Cifuentes, Th. Henning, A. Kaminski, R. Luque, D. Montes, J. C. Morales, S. Pedraz, H. M. Tabernero, M. Zechmeister
The large amounts of astrophysical data being provided by existing and future instrumentation require efficient and fast analysis tools. Transfer learning is a new technique promising higher accuracy in the derived data products, with information fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7a3da2f8fac391d6e312be5ead9b095
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. Suárez Mascareño, E. González-Álvarez, M. R. Zapatero Osorio, J. Lillo-Box, J. P. Faria, V. M. Passegger, J. I. González Hernández, P. Figueira, A. Sozzetti, R. Rebolo, F. Pepe, N. C. Santos, S. Cristiani, C. Lovis, A. M. Silva, I. Ribas, P. J. Amado, J. A. Caballero, A. Quirrenbach, A. Reiners, M. Zechmeister, V. Adibekyan, Y. Alibert, V. J. S. Béjar, S. Benatti, V. D’Odorico, M. Damasso, J.-B. Delisle, P. Di Marcantonio, S. Dreizler, D. Ehrenreich, A. P. Hatzes, N. C. Hara, Th. Henning, A. Kaminski, M. J. López-González, C. J. A. P. Martins, G. Micela, D. Montes, E. Pallé, S. Pedraz, E. Rodríguez, C. Rodríguez-López, L. Tal-Or, S. Sousa, S. Udry
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1584dc6c075fb22abc8242da3c89c47f
http://arxiv.org/abs/2212.07332
http://arxiv.org/abs/2212.07332
Autor:
A. Quirrenbach, V. M. Passegger, T. Trifonov, P. J. Amado, J. A. Caballero, A. Reiners, I. Ribas, J. Aceituno, V. J. S. Béjar, P. Chaturvedi, L. González-Cuesta, T. Henning, E. Herrero, A. Kaminski, M. Kürster, S. Lalitha, N. Lodieu, M. J. López-González, D. Montes, E. Pallé, M. Perger, D. Pollacco, S. Reffert, E. Rodríguez, C. Rodríguez López, Y. Shan, L. Tal-Or, M. R. Zapatero Osorio, M. Zechmeister
The CARMENES radial-velocity survey is currently searching for planets in a sample of 387 M dwarfs. Here we report on two Saturn-mass planets orbiting TYC 2187-512-1 (M* = 0.50 M⊙) and TZ Ari (M* = 0.15 M⊙), respectively. We obtained supplementar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02c57c6b0f646e4456743565d5fbbe56
http://arxiv.org/abs/2203.16504
http://arxiv.org/abs/2203.16504