Zobrazeno 1 - 10
of 299
pro vyhledávání: '"S. Pedraz"'
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:
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, 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:
J. Lillo-Box, N. C. Santos, A. Santerne, A. M. Silva, D. Barrado, J. Faria, A. Castro-González, O. Balsalobre-Ruza, M. Morales-Calderón, A. Saavedra, E. Marfil, S. G. Sousa, V. Adibekyan, A. Berihuete, S. C. C. Barros, E. Delgado-Mena, N. Huélamo, M. Deleuil, O. D. S. Demangeon, P. Figueira, S. Grouffal, J. Aceituno, M. Azzaro, G. Bergond, A. Fernández-Martín, D. Galadí, E. Gallego, A. Gardini, S. Góngora, A. Guijarro, I. Hermelo, P. Martín, P. Mínguez, L. M. Montoya, S. Pedraz, J. I. Vico Linares
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 667, ⟨10.1051/0004-6361/202243898⟩
Astronomy and Astrophysics-A&A, 2022, 667, ⟨10.1051/0004-6361/202243898⟩
The detection of habitable worlds is one of humanity's greatest endeavors. So far, astrobiological studies show that one of the most critical components for life development is liquid water. Its chemical properties and its capacity to dissolve and he
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1a9a8760ac8089925b95ef5fdd0adea6
http://arxiv.org/abs/2209.05205
http://arxiv.org/abs/2209.05205
Autor:
V. M. Passegger, A. Bello-García, J. Ordieres-Meré, A. Antoniadis-Karnavas, E. Marfil, C. Duque-Arribas, P. J. Amado, E. Delgado-Mena, D. Montes, B. Rojas-Ayala, A. Schweitzer, H. M. Tabernero, V. J. S. Béjar, J. A. Caballero, A. P. Hatzes, Th. Henning, S. Pedraz, A. Quirrenbach, A. Reiners, I. Ribas
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
Deriving metallicities for solar-like stars follows well-established methods, but for cooler stars such as M dwarfs, the determination is much more complicated due to forests of molecular lines that are present. Several methods have been developed in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::733f382913b372aec9bc0e49950ddc76
https://eprints.ucm.es/id/eprint/74773/1/gomezmarfil06preprint.pdf
https://eprints.ucm.es/id/eprint/74773/1/gomezmarfil06preprint.pdf
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⟩
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ba458833ec3178b310d5589782d8d47
Autor:
E. González-Álvarez, M. R. Zapatero Osorio, J. Sanz-Forcada, J. A. Caballero, S. Reffert, V. J. S. Béjar, A. P. Hatzes, E. Herrero, S. V. Jeffers, J. Kemmer, M. J. López-González, R. Luque, K. Molaverdikhani, G. Morello, E. Nagel, A. Quirrenbach, E. Rodríguez, C. Rodríguez-López, M. Schlecker, A. Schweitzer, S. Stock, V. M. Passegger, T. Trifonov, P. J. Amado, D. Baker, P. T. Boyd, C. Cadieux, D. Charbonneau, K. A. Collins, R. Doyon, S. Dreizler, N. Espinoza, G. Fűrész, E. Furlan, K. Hesse, S. B. Howell, J. M. Jenkins, R. C. Kidwell, D. W. Latham, K. K. McLeod, D. Montes, J. C. Morales, T. O’Dwyer, E. Pallé, S. Pedraz, A. Reiners, I. Ribas, S. N. Quinn, C. Schnaible, S. Seager, B. Skinner, J. C. Smith, R. P. Schwarz, A. Shporer, R. Vanderspek, J. N. Winn
Publikováno v:
Astronomy and Astrophysics
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
Context. The number of super-Earth and Earth-mass planet discoveries has increased significantly in the last two decades thanks to the Doppler radial velocity and planetary transit observing techniques. Either technique can detect planet candidates o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::348ced6c149f3c767c8433ccefaad0ba
https://hdl.handle.net/21.11116/0000-000C-B1B6-E
https://hdl.handle.net/21.11116/0000-000C-B1B6-E
Autor:
D. Cont, F. Yan, A. Reiners, L. Nortmann, K. Molaverdikhani, E. Pallé, Th. Henning, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, S. Czesla, F. Lesjak, M. López-Puertas, P. Mollière, D. Montes, G. Morello, E. Nagel, S. Pedraz, A. Sánchez-López
Publikováno v:
Astronomy & Astrophysics, 668:A53
Ultra-hot Jupiters are highly irradiated gas giant exoplanets on close-in orbits around their host stars. We analyzed high-resolution spectra from CARMENES, HARPS-N, and ESPaDOnS taken over eight observation nights to study the emission spectrum of W
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f67b64836c2c72ce454c1933001c2610
Autor:
J. A. Caballero, E. González-Álvarez, M. Brady, T. Trifonov, T. G. Ellis, C. Dorn, C. Cifuentes, K. Molaverdikhani, J. L. Bean, T. Boyajian, E. Rodríguez, J. Sanz-Forcada, M. R. Zapatero Osorio, C. Abia, P. J. Amado, N. Anugu, V. J. S. Béjar, C. L. Davies, S. Dreizler, F. Dubois, J. Ennis, N. Espinoza, C. D. Farrington, A. García López, T. Gardner, A. P. Hatzes, Th. Henning, E. Herrero, E. Herrero-Cisneros, A. Kaminski, D. Kasper, R. Klement, S. Kraus, A. Labdon, C. Lanthermann, J.-B. Le Bouquin, M. J. López González, R. Luque, A. W. Mann, E. Marfil, J. D. Monnier, D. Montes, J. C. Morales, E. Pallé, S. Pedraz, A. Quirrenbach, S. Reffert, A. Reiners, I. Ribas, C. Rodríguez-López, G. Schaefer, A. Schweitzer, A. Seifahrt, B. R. Setterholm, Y. Shan, D. Shulyak, E. Solano, K. R. Sreenivas, G. Stefánsson, J. Stürmer, H. M. Tabernero, L. Tal-Or, T. ten Brummelaar, S. Vanaverbeke, K. von Braun, A. Youngblood, M. Zechmeister
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Context. The Gl 486 system consists of a very nearby, relatively bright, weakly active M3.5 V star at just 8 pc with a warm transiting rocky planet of about 1.3 R-circle plus and 3.0 M-circle plus. It is ideal for both transmission and emission spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24d5e79c0d266fc71a636292a0135060
http://hdl.handle.net/10852/101335
http://hdl.handle.net/10852/101335