Zobrazeno 1 - 10
of 1 301
pro vyhledávání: '"Puertas M"'
Publikováno v:
Journal of Supercomputing 78, pp. 17826-17843, 2022
The computation of the domination-type parameters is a challenging problem in Cartesian product graphs. We present an algorithmic method to compute the $2$-domination number of the Cartesian product of a path with small order and any cycle, involving
Externí odkaz:
http://arxiv.org/abs/2409.17688
Publikováno v:
IEEE Access, vol. 9, pp. 29346-29355, 2021
The Roman domination in a graph $G$ is a variant of the classical domination, defined by means of a so-called Roman domination function $f\colon V(G)\to \{0,1,2\}$ such that if $f(v)=0$ then, the vertex $v$ is adjacent to at least one vertex $w$ with
Externí odkaz:
http://arxiv.org/abs/2409.17658
Autor:
Masson, A., Vinatier, S., Bézard, B., López-Puertas, M., Lampón, M., Debras, F., Carmona, A., Klein, B., Artigau, E., Dethier, W., Pelletier, S., Hood, T., Allart, R., Bourrier, V., Cadieux, C., Charnay, B., Cowan, N. B., Cook, N. J., Delfosse, X., Donati, J. -F., Gu, P. -G., Hébrard, G., Martioli, E., Moutou, C., Venot, O., Wyttenbach, A.
For several years, the metastable helium triplet line has been successfully used as a tracer to probe atmospheric escape in transiting exoplanets. This absorption in the near-infrared (1083.3 nm) can be observed from the ground using high-resolution
Externí odkaz:
http://arxiv.org/abs/2406.09225
Autor:
Guo, B., Yan, F., Nortmann, L., Cont, D., Reiners, A., Pallé, E., Shulyak, D., Molaverdikhani, K., Henning, Th., Chen, G., Stangret, M., Czesla, S., Lesjak, F., López-Puertas, M., Ribas, I., Quirrenbach, A., Caballero, J. A., Amado, P. J., Blazek, M., Montes, D., Morales, J. C., Nagel, E., Osorio, M. R. Zapatero
Ultrahot Jupiters are a type of gaseous exoplanet that orbit extremely close to their host star, resulting in significantly high equilibrium temperatures. In recent years, high-resolution emission spectroscopy has been broadly employed in observing t
Externí odkaz:
http://arxiv.org/abs/2404.18788
Autor:
Orell-Miquel, J., Murgas, F., Pallé, E., Mallorquín, M., López-Puertas, M., Lampón, M., Sanz-Forcada, J., Nortmann, L., Czesla, S., Nagel, E., Ribas, I., Stangret, M., Livingston, J., Knudstrup, E., Albrecht, S. H., Carleo, I., Caballero, J., Dai, F., Esparza-Borges, E., Fukui, A., Heng, K., Henning, Th., Kagetani, T., Lesjak, F., de Leon, J. P., Montes, D., Morello, G., Narita, N., Quirrenbach, A., Amado, P. J., Reiners, A., Schweitzer, A., Linares, J. I. Vico
Publikováno v:
A&A 689, A179 (2024)
During the first Gyr of their life, exoplanet atmospheres suffer from different atmospheric escape phenomena that can strongly affect the shape and morphology of the exoplanet itself. These processes can be studied with Ly$\alpha$, H$\alpha$ and/or H
Externí odkaz:
http://arxiv.org/abs/2404.16732
Autor:
Czesla, S., Lampón, M., Cont, D., Lesjak, F., Orell-Miquel, J., Sanz-Forcada, J., Nagel, E., Nortmann, L., Molaverdikhani, K., López-Puertas, M., Yan, F., Quirrenbach, A., Caballero, J. A., Pallé, E., Aceituno, J., Amado, P. J., Henning, Th., Khalafinejad, S., Montes, D., Reiners, A., Ribas, I., Schweitzer, A.
To date, the hot Jupiter WASP-12 b has been the only planet with confirmed orbital decay. The late F-type host star has been hypothesized to be surrounded by a large structure of circumstellar material evaporated from the planet. We obtained two high
Externí odkaz:
http://arxiv.org/abs/2401.02195
Autor:
Nagel, E., Czesla, S., Kaminski, A., Zechmeister, M., Tal-Or, L., Schmitt, J. H. M. M., Reiners, A., Quirrenbach, A., López, A. García, Caballero, J. A., Ribas, I., Amado, P. J., Béjar, V. J. S., Cortés-Contreras, M., Dreizler, S., Hatzes, A. P., Henning, Th., Jeffers, S. V., Kürster, M., Lafarga, M., López-Puertas, M., Montes, D., Morales, J. C., Pedraz, S., Schweitzer, A.
Publikováno v:
A&A 680, A73 (2023)
Light from celestial objects interacts with the molecules of the Earth's atmosphere, resulting in the production of telluric absorption lines in ground-based spectral data. Correcting for these lines, which strongly affect red and infrared wavelength
Externí odkaz:
http://arxiv.org/abs/2310.14715
Autor:
Orell-Miquel, J., Lampón, M., López-Puertas, M., Mallorquín, M., Murgas, F., Peláez-Torres, A., Pallé, E., Esparza-Borges, E., Sanz-Forcada, J., Tabernero, H. M., Nortmann, L., Nagel, E., Parviainen, H., Osorio, M. R. Zapatero, Caballero, J. A., Czesla, S., Cifuentes, C., Morello, G., Quirrenbach, A., Amado, P. J., Fernández-Martín, A., Fukui, A., Henning, Th., Kawauchi, K., de Leon, J. P., Molaverdikhani, K., Montes, D., Narita, N., Reiners, A., Ribas, I., Sánchez-López, A., Schweitzer, A., Stangret, M., Yan, F.
Publikováno v:
A&A 677, A56 (2023)
HD235088 (TOI-1430) is a young star known to host a sub-Neptune-sized planet candidate. We validated the planetary nature of HD235088 b with multiband photometry, refined its planetary parameters, and obtained a new age estimate of the host star, pla
Externí odkaz:
http://arxiv.org/abs/2307.05191
Autor:
Lampón, M., López-Puertas, M., Sanz-Forcada, J., Czesla, S., Nortmann, L., Casasayas-Barris, N., Orell-Miquel, J., Sánchez-López, A., Danielski, C., Pallé, E., Molaverdikhani, K., Henning, Th., Caballero, J. A., Amado, P. J., Quirrenbach, A., Reiners, A., Ribas, I.
Publikováno v:
A&A 673, A140 (2023)
Characterisation of atmospheres undergoing photo-evaporation is key to understanding the formation, evolution, and diversity of planets. However, only a few upper atmospheres that experience this kind of hydrodynamic escape have been characterised. O
Externí odkaz:
http://arxiv.org/abs/2304.03839
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