Zobrazeno 1 - 10
of 50
pro vyhledávání: '"S. Khalafinejad"'
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. Orell-Miquel, F. Murgas, E. Pallé, M. Lampón, M. López-Puertas, J. Sanz-Forcada, E. Nagel, A. Kaminski, N. Casasayas-Barris, L. Nortmann, R. Luque, K. Molaverdikhani, E. Sedaghati, J. A. Caballero, P. J. Amado, G. Bergond, S. Czesla, A. P. Hatzes, Th. Henning, S. Khalafinejad, D. Montes, G. Morello, A. Quirrenbach, A. Reiners, I. Ribas, A. Sánchez-López, A. Schweitzer, M. Stangret, F. Yan, M. R. Zapatero Osorio
Publikováno v:
Astronomy & Astrophysics, 659:A55
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
The He I λ10833 Å triplet is a powerful tool for characterising the upper atmosphere of exoplanets and tracing possible mass loss. Here, we analysed one transit of GJ 1214 b observed with the CARMENES high-resolution spectrograph to study its atmo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::965cfced78f3b58a47e55efeeb731ae2
http://hdl.handle.net/10261/272229
http://hdl.handle.net/10261/272229
Autor:
R. Luque, B. J. Fulton, M. Kunimoto, P. J. Amado, P. Gorrini, S. Dreizler, C. Hellier, G. W. Henry, K. Molaverdikhani, G. Morello, L. Peña-Moñino, M. Pérez-Torres, F. J. Pozuelos, Y. Shan, G. Anglada-Escudé, V. J. S. Béjar, G. Bergond, A. W. Boyle, J. A. Caballero, D. Charbonneau, D. R. Ciardi, S. Dufoer, N. Espinoza, M. Everett, D. Fischer, A. P. Hatzes, Th. Henning, K. Hesse, A. W. Howard, S. B. Howell, H. Isaacson, S. V. Jeffers, J. M. Jenkins, S. R. Kane, J. Kemmer, S. Khalafinejad, R. C. Kidwell, D. Kossakowski, D. W. Latham, J. Lillo-Box, J. J. Lissauer, D. Montes, J. Orell-Miquel, E. Pallé, D. Pollacco, A. Quirrenbach, S. Reffert, A. Reiners, I. Ribas, G. R. Ricker, L. A. Rogers, J. Sanz-Forcada, M. Schlecker, A. Schweitzer, S. Seager, A. Shporer, K. G. Stassun, S. Stock, L. Tal-Or, E. B. Ting, T. Trifonov, S. Vanaverbeke, R. Vanderspek, J. Villaseñor, J. N. Winn, J. G. Winters, M. R. Zapatero Osorio
Publikováno v:
Astronomy and Astrophysics
Full list of authors: Luque, R.; Fulton, B. J.; Kunimoto, M.; Amado, P. J.; Gorrini, P.; Dreizler, S.; Hellier, C.; Henry, G. W.; Molaverdikhani, K.; Morello, G.; Pena-Monino, L.; Perez-Torres, M.; Pozuelos, F. J.; Shan, Y.; Anglada-Escude, G.; Bejar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc651c860d1295e825dd278d64d53a2d
http://hdl.handle.net/10852/101330
http://hdl.handle.net/10852/101330
Autor:
F. Yan, A. Reiners, E. Pallé, D. Shulyak, M. Stangret, K. Molaverdikhani, L. Nortmann, P. Mollière, Th. Henning, N. Casasayas-Barris, D. Cont, G. Chen, S. Czesla, A. Sánchez-López, M. López-Puertas, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, D. Galadí-Enríquez, S. Khalafinejad, L. M. Lara, D. Montes, G. Morello, E. Nagel, E. Sedaghati, M. R. Zapatero Osorio, M. Zechmeister
Publikováno v:
Astronomy and Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Astronomy & Astrophysics, 659:A7
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Astronomy & Astrophysics, 659:A7
Ultra-hot Jupiters (UHJs) are gas giants with very high equilibrium temperatures. In recent years, multiple chemical species, including various atoms and ions, have been discovered in their atmospheres. Most of these observations have been performed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::03dcd86c915a216060e4dcee85c5b118
https://hdl.handle.net/1887/3515371
https://hdl.handle.net/1887/3515371
Akademický článek
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Publikováno v:
Astronomy & Astrophysics
Autor:
S. Khalafinejad, K. Molaverdikhani, J. Blecic, M. Mallonn, L. Nortmann, J. A. Caballero, H. Rahmati, A. Kaminski, S. Sadegi, E. Nagel, L. Carone, P. J. Amado, M. Azzaro, F. F. Bauer, N. Casasayas-Barris, S. Czesla, C. von Essen, L. Fossati, M. Güdel, Th. Henning, M. López-Puertas, M. Lendl, T. Lüftinger, D. Montes, M. Oshagh, E. Pallé, A. Quirrenbach, S. Reffert, A. Reiners, I. Ribas, S. Stock, F. Yan, M. R. Zapatero Osorio, M. Zechmeister
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
Khalafinejad, S, Molaverdikhani, K, Blecic, J, Mallonn, M, Nortmann, L, Caballero, J A, Rahmati, H, Kaminski, A, Sadegi, S, Nagel, E, Carone, L, Amado, P J, Azzaro, M, Bauer, F F, Casasayas-Barris, N, Czesla, S, Von Essen, C, Fossati, L, Güdel, M, Henning, T, López-Puertas, M, Lendl, M, Lüftinger, T, Montes, D, Oshagh, M, Pallé, E, Quirrenbach, A, Reffert, S, Reiners, A, Ribas, I, Stock, S, Yan, F, Zapatero Osorio, M R & Zechmeister, M 2021, ' Probing the atmosphere of WASP-69 b with low-and high-resolution transmission spectroscopy ', Astronomy and Astrophysics, vol. 656, A142 . https://doi.org/10.1051/0004-6361/202141191
Digital.CSIC. Repositorio Institucional del CSIC
Monthly Notices of the Royal Astronomical Society, 656, 1-20
instname
Khalafinejad, S, Molaverdikhani, K, Blecic, J, Mallonn, M, Nortmann, L, Caballero, J A, Rahmati, H, Kaminski, A, Sadegi, S, Nagel, E, Carone, L, Amado, P J, Azzaro, M, Bauer, F F, Casasayas-Barris, N, Czesla, S, Von Essen, C, Fossati, L, Güdel, M, Henning, T, López-Puertas, M, Lendl, M, Lüftinger, T, Montes, D, Oshagh, M, Pallé, E, Quirrenbach, A, Reffert, S, Reiners, A, Ribas, I, Stock, S, Yan, F, Zapatero Osorio, M R & Zechmeister, M 2021, ' Probing the atmosphere of WASP-69 b with low-and high-resolution transmission spectroscopy ', Astronomy and Astrophysics, vol. 656, A142 . https://doi.org/10.1051/0004-6361/202141191
Digital.CSIC. Repositorio Institucional del CSIC
Monthly Notices of the Royal Astronomical Society, 656, 1-20
Consideration of both low- and high-resolution transmission spectroscopy is key for obtaining a comprehensive picture of exoplanet atmospheres. In studies of transmission spectra, the continuum information is well established with low-resolution spec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fed7d5ad32d5ea816c13479b382176c4
https://eprints.ucm.es/id/eprint/72728/1/davidmontes135preprint.pdf
https://eprints.ucm.es/id/eprint/72728/1/davidmontes135preprint.pdf
Autor:
J. Orell-Miquel, Jose A. Caballero, G. Bergond, Rafael Luque, S. Khalafinejad, Lisa Nortmann, Andreas Quirrenbach, S. Czesla, Fei Yan, Mathias Zechmeister, G. Morello, Pedro J. Amado, K. Molaverdikhani, Evangelos Nagel, Enric Palle, Manuel López-Puertas, Elyar Sedaghati, Ignas Snellen, N. Casasayas-Barris, M. Stangret, Mahmoudreza Oshagh, D. Montes, A. Sánchez-López, Jorge Sanz-Forcada, Manuel Perger, Ignasi Ribas, Th. Henning, Ansgar Reiners
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Astronomy and Astrophysics, 654
instname
E-Prints Complutense. Archivo Institucional de la UCM
Astronomy and Astrophysics, 654
Casasayas-Barris, N., et al.
Ultra-hot Jupiters are highly irradiated gas giants with equilibrium temperatures typically higher than 2000 K. Atmospheric studies of these planets have shown that their transmission spectra are rich in metal lines,
Ultra-hot Jupiters are highly irradiated gas giants with equilibrium temperatures typically higher than 2000 K. Atmospheric studies of these planets have shown that their transmission spectra are rich in metal lines,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31694bf744895d4224be2e14228349df
http://hdl.handle.net/10261/260110
http://hdl.handle.net/10261/260110
Autor:
S. Czesla, M. Lampón, J. Sanz-Forcada, A. García Muñoz, M. López-Puertas, L. Nortmann, D. Yan, E. Nagel, F. Yan, J. H. M. M. Schmitt, J. Aceituno, P. J. Amado, J. A. Caballero, N. Casasayas-Barris, Th. Henning, S. Khalafinejad, K. Molaverdikhani, D. Montes, E. Pallé, A. Reiners, P. C. Schneider, I. Ribas, A. Quirrenbach, M. R. Zapatero Osorio, M. Zechmeister
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
We analyze two high-resolution spectral transit time series of the hot Jupiter HAT-P-32 b obtained with the CARMENES spectrograph. Our new XMM-Newton X-ray observations of the system show that the fast-rotating F-type host star exhibits a high X-ray
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46aebb5898dd44b9f50805a414e039fc
https://eprints.ucm.es/id/eprint/72723/1/davidmontes134preprint.pdf
https://eprints.ucm.es/id/eprint/72723/1/davidmontes134preprint.pdf
Autor:
Matthias Mallonn, Gražina Tautvaišienė, Keivan G. Stassun, C. C. Borre, S. Khalafinejad, Victoria Antoci, C. von Essen
Publikováno v:
Von Essen, C, Mallonn, M, Borre, C C, Antoci, V, Stassun, K G, Khalafinejad, S & Tautvaišienė, G 2020, ' TESS unveils the phase curve of WASP-33b : Characterization of the planetary atmosphere and the pulsations from the star ', Astronomy and Astrophysics, vol. 639, A34 . https://doi.org/10.1051/0004-6361/202037905
Von Essen, C, Mallonn, M, Borre, C C, Antoci, V, Stassun, K G, Khalafinejad, S & Tautvaišienė, G 2020, ' TESS unveils the phase curve of WASP-33b: Characterization of the planetary atmosphere and the pulsations from the star ', Astronomy and Astrophysics, vol. 639, A34 . https://doi.org/10.1051/0004-6361/202037905
Von Essen, C, Mallonn, M, Borre, C C, Antoci, V, Stassun, K G, Khalafinejad, S & Tautvaišienė, G 2020, ' TESS unveils the phase curve of WASP-33b: Characterization of the planetary atmosphere and the pulsations from the star ', Astronomy and Astrophysics, vol. 639, A34 . https://doi.org/10.1051/0004-6361/202037905
We present the detection and characterization of the full-orbit phase curve and secondary eclipse of the ultra-hot Jupiter WASP-33b at optical wavelengths, along with the pulsation spectrum of the host star. We analyzed data collected by the Transiti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fbf78c81bf4c3e531ab1fd3b6b0f402e
https://pure.au.dk/portal/da/publications/tess-unveils-the-phase-curve-of-wasp33b(49b5db9e-cfa6-408c-aa3f-96c89681baa5).html
https://pure.au.dk/portal/da/publications/tess-unveils-the-phase-curve-of-wasp33b(49b5db9e-cfa6-408c-aa3f-96c89681baa5).html