Zobrazeno 1 - 10
of 668
pro vyhledávání: '"Azzaro, M"'
Autor:
Pérez, I., Verley, S., Sánchez-Menguiano, L., Ruiz-Lara, T., García-Benito, R., Puertas, S. Duarte, Jiménez, A., Domínguez-Gómez, J., Espada, D., Peletier, R. F., Román, J., Rodríguez, M. I., Alarcón, P. Sánchez, Argudo-Fernández, M., Torres-Ríos, G., Bidaran, B., Alcázar-Laynez, M., van de Weygaert, R., Sánchez, S. F., Lisenfeld, U., Zurita, A., Florido, E., van der Hulst, J. M., Blázquez-Calero, G., Villalba-González, P., del Moral-Castro, I., Lugo-Aranda, A., Walo-Martín, D., Conrado, A., Delgado, R. González, Falcón-Barroso, J., Ferré-Mateu, A., Hernández-Sánchez, M., Awad, P., Kreckel, K., Courtois, H., Espada-Miura, R., Relaño, M., Galbany, L., Sánchez-Blázquez, P., Pérez-Montero, E., Sánchez-Portal, M., Bongiovanni, A., Planelles, S., Quilis, V., Aubert, M., Guinet, D., Pomaréde, D., Weijmans, A. M., Raj, M. A., Aragón-Calvo, M. A., Azzaro, M., Bergond, G., Blazek, M., Cikota, S., Fernández-Martín, A., Gardini, A., Guijarro, A., Hermelo, I., Martín, P., Linares, J. I. Vico
We have learnt in the last decades that the majority of galaxies belong to high density regions interconnected in a sponge-like fashion. This large-scale structure is characterised by clusters, filaments, walls, where most galaxies concentrate, but a
Externí odkaz:
http://arxiv.org/abs/2405.04217
Autor:
Murgas, F., Pallé, E., Orell-Miquel, J., Carleo, I., Peña-Moñino, L., Pérez-Torres, M., Watkins, C. N., Jeffers, S. V., Azzaro, M., Barkaoui, K., Belinski, A. A., Caballero, J. A., Charbonneau, D., Cheryasov, D. V., Ciardi, D. R., Collins, K. A., Cortés-Contreras, M., de Leon, J., Duque-Arribas, C., Enoc, G., Esparza-Borges, E., Fukui, A., Geraldía-González, S., Gilbert, E. A., Hatzes, A. P., Hayashi, Y., Henning, Th., Herrero, E., Jenkins, J. M., Lillo-Box, J., Lodieu, N., Lund, M. B., Luque, R., Montes, D., Nagel, E., Narita, N., Parviainen, H., Polanski, A. S., Reffert, S., Schlecker, M., Schöfer, P., Schwarz, R. P., Schweitzer, A., Seager, S., Stassun, K. G., Tabernero, H. M., Terada, Y., Twicken, J. D., Vanaverbeke, S., Winn, J. N., Zambelli, R., Amado, P. J., Quirrenbach, A., Reiners, A., Ribas, I.
Planets with orbital periods shorter than 1 day are rare and have formation histories that are not completely understood. Small ($R_\mathrm{p} < 2\; R_\oplus$) ultra-short-period (USP) planets are highly irradiated, probably have rocky compositions w
Externí odkaz:
http://arxiv.org/abs/2401.12150
Autor:
Ribas, I., Reiners, A., Zechmeister, M., Caballero, J. A., Morales, J. C., Sabotta, S., Baroch, D., Amado, P. J., Quirrenbach, A., Abril, M., Aceituno, J., Anglada-Escudé, G., Azzaro, M., Barrado, D., Béjar, V. J. S., de Haro, D. Benítez, Bergond, G., Bluhm, P., Ortega, R. Calvo, Guillén, C. Cardona, Chaturvedi, P., Cifuentes, C., Colomé, J., Cont, D., Cortés-Contreras, M., Czesla, S., Díez-Alonso, E., Dreizler, S., Duque-Arribas, C., Espinoza, N., Fernández, M., Fuhrmeister, B., Galadí-Enríquez, D., García-López, A., González-Álvarez, E., Hernández, J. I. González, Guenther, E. W., de Guindos, E., Hatzes, A. P., Henning, Th., Herrero, E., Hintz, D., Huelmo, Á. L., Jeffers, S. V., Johnson, E. N., de Juan, E., Kaminski, A., Kemmer, J., Khaimova, J., Khalafinejad, S., Kossakowski, D., Kürster, M., Labarga, F., Lafarga, M., Lalitha, S., Lampón, M., Lillo-Box, J., Lodieu, N., González, M. J. López, López-Puertas, M., Luque, R., Magán, H., Mancini, L., Marfil, E., Martín, E. L., Martín-Ruiz, S., Molaverdikhani, K., Montes, D., Nagel, E., Nortmann, L., Nowak, G., Pallé, E., Passegger, V. M., Pavlov, A., Pedraz, S., Perdelwitz, V., Perger, M., Ramón-Ballesta, A., Reffert, S., Revilla, D., Rodríguez, E., Rodríguez-López, C., Sadegi, S., Carrasco, M. Á. Sánchez, Sánchez-López, A., Sanz-Forcada, J., Schäfer, S., Schlecker, M., Schmitt, J. H. M. M., Schöfer, P., Schweitzer, A., Seifert, W., Shan, Y., Skrzypinski, S. L., Solano, E., Stahl, O., Stangret, M., Stock, S., Stürmer, J., Tabernero, H. M., Tal-Or, L., Trifonov, T., Vanaverbeke, S., Yan, F., Osorio, M. R. Zapatero
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:
http://arxiv.org/abs/2302.10528
The CARMENES search for exoplanets around M dwarfs. Line-by-line sensitivity to activity in M dwarfs
Autor:
Lafarga, M., Ribas, I., Zechmeister, M., Reiners, A., López-Gallifa, Á., Montes, D., Quirrenbach, A., Amado, P. J., Caballero, J. A., Azzaro, M., Béjar, V. J. S., Hatzes, A. P., Henning, Th., Jeffers, S. V., Kaminski, A., Kürster, M., Schöfer, P., Schweitzer, A., Tabernero, H. M., Osorio, M. R. Zapatero
Publikováno v:
A&A 674, A61 (2023)
Radial velocities (RVs) measured from high-resolution stellar spectra are routinely used to detect and characterise orbiting exoplanet companions. The different lines present in stellar spectra are created by several species, which are non-uniformly
Externí odkaz:
http://arxiv.org/abs/2302.07916
Autor:
Balsalobre-Ruza, O., Lillo-Box, J., Berihuete, A., Silva, A. M., Santos, N. C., Castro-González, A., Faria, J. P., Huélamo, N., Barrado, D., Demangeon, O. D. S., Marfil, E., Aceituno, J., Adibekyan, V., Azzaro, M., Barros, S. C. C., Bergond, G., Galadí-Enríquez, D., Pedraz, S., Santerne, A.
Ground-based observing time is precious in the era of exoplanet follow-up and characterization, especially in high-precision radial velocity instruments. Blind-search radial velocity surveys thus require a dedicated observational strategy in order to
Externí odkaz:
http://arxiv.org/abs/2210.11207
Autor:
Lillo-Box, J., Santos, N. C., Santerne, A., Silva, A. M., Barrado, D., Faria, J., Castro-González, A., Balsalobre-Ruza, O., Morales-Calderón, M., Saavedra, A., Marfil, E., Sousa, S. G., Adibekyan, V., Berihuete, A., Barros, S. C. C., Delgado-Mena, E., Huélamo, N., Deleuil, M., Demangeon, O. D. S., Figueira, P., Grouffal, S., Aceituno, J., Azzaro, M., Bergond, G., Fernández-Martín, A., Galadí, D., Gallego, E., Gardini, A., Góngora, S., Guijarro, A., Hermelo, I., Martín, P., Mínguez, P., Montoya, L. M., Pedraz, S., Linares, J. I. Vico
Publikováno v:
A&A 667, A102 (2022)
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:
http://arxiv.org/abs/2209.05205
Autor:
Reiners, A., Shulyak, D., Käpylä, P. J., Ribas, I., Nagel, E., Zechmeister, M., Caballero, J. A., Shan, Y., Fuhrmeister, B., Quirrenbach, A., Amado, P. J., Montes, D., Jeffers, S. V., Azzaro, M., Béjar, V. J. S., Chaturvedi, P., Henning, Th., Kürster, M., Pallé, E.
Publikováno v:
A&A 662, A41 (2022)
Stellar dynamos generate magnetic fields that are of fundamental importance to the variability and evolution of Sun-like and low-mass stars, and for the development of their planetary systems. We report measurements of surface-average magnetic fields
Externí odkaz:
http://arxiv.org/abs/2204.00342
Autor:
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, Th., 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., Osorio, M. R. Zapatero, Zechmeister, M.
Publikováno v:
A&A 656, A142 (2021)
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:
http://arxiv.org/abs/2109.06335
Autor:
Sabotta, S., Schlecker, M., Chaturvedi, P., Guenther, E. W., Rodríguez, I. Muñoz, Sánchez, J. C. Muñoz, Caballero, J. A., Shan, Y., Reffert, S., Ribas, I., Reiners, A., Hatzes, A. P., Amado, P. J., Klahr, H., Morales, J. C., Quirrenbach, A., Henning, Th., Dreizler, S., Pallé, E., Perger, M., Azzaro, M., Jeffers, S. V., Kaminski, A., Kürster, M., Lafarga, M., Montes, D., Passegger, V. M., Zechmeister, M.
Publikováno v:
A&A 653, A114 (2021)
The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 nearby M dwarfs over the past five years as part of its guaranteed time observations (GTO) program. We determine planet occurrence rates with the 71 stars from the
Externí odkaz:
http://arxiv.org/abs/2107.03802
Autor:
Amado, P. J., Bauer, F. F., López, C. Rodríguez, Rodríguez, E., Guillén, C. Cardona, Perger, M., Caballero, J. A., López-González, M. J., Rodríguez, I. Muñoz, Pozuelos, F. J., Sánchez-Rivero, A., Schlecker, M., Quirrenbach, A., Ribas, I., Reiners, A., Almenara, J., Astudillo-Defru, N., Azzaro, M., Béjar, V. J. S., Bohemann, R., Bonfils, X., Bouchy, F., Cifuentes, C., Cortés-Contreras, M., Delfosse, X., Dreizler, S., Forveille, T., Hatzes, A. P., Henning, Th., Jeffers, S. V., Kaminski, A., Kürster, M., Lafarga, M., Lodieu, N., Lovis, C., Mayor, M., Montes, D., Morales, J. C., Morales, N., Murgas, F., Ortiz, J. L., Pepe, F., Perdelwitz, V., Pollaco, D., Santos, N. C., Schöfer, P., Schweitzer, A., Ségransan, N. C., Shan, Y., Stock, S., Tal-Or, L., Udry, S., Osorio, M. R. Zapatero, Zechmeister, M.
Publikováno v:
A&A 650, A188 (2021)
We report the discovery of two planetary systems, namely G 264-012, an M4.0 dwarf with two terrestrial planets ($M_{\rm b}\sin{i} = 2.50^{+0.29}_{-0.30}$ M$_{\oplus}$ and $M_{\rm c}\sin{i} = 3.75^{+0.48}_{-0.47}$ M$_{\oplus}$), and Gl 393, a bright M
Externí odkaz:
http://arxiv.org/abs/2105.13785