Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Murabito, S."'
Autor:
Vaduvescu, O., Hudin, L., Mocnik, T., Char, F., Sonka, A., Tudor, V., Ordonez-Etxeberria, I., Alfaro, M. Diaz, Ashley, R., Errmann, R., Short, P., Moloceniuc, A., Cornea, R., Inceu, V., Zavoianu, D., Popescu, M., Curelaru, L., Mihalea, S., Stoian, A. -M., Boldea, A., Toma, R., Fields, L., Grigore, V., Stoev, H., Lopez-Martinez, F., Humphries, N., Sowicka, P., Ramanjooloo, Y., Manilla-Robles, A., Riddick, F. C., Jimenez-Lujan, F., Mendez, J., Aceituno, F., Sota, A., Jones, D., Hidalgo, S., Murabito, S., Oteo, I., Bongiovanni, A., Zamora, O., Pyrzas, S., Genova-Santos, R., Font, J., Bereciartua, A., Perez-Fournon, I., Martinez-Vazquez, C. E., Monelli, M., Cicuendez, L., Monteagudo, L., Agulli, I., Bouy, H., Huelamo, N., Monguio, M., Gansicke, B. T., Steeghs, D., Gentile-Fusillo, N. P., Hollands, M. A., Toloza, O., Manser, C. J., Dhillon, V., Sahman, D., Fitzsimmons, A., McNeill, A., Thompson, A., Tabor, M., Murphy, D. N. A., Davies, J., Snodgrass, C., Triaud, A. H. M. J., Groot, P. J., Macfarlane, S., Peletier, R., Sen, S., Ikiz, T., Hoekstra, H., Herbonnet, R., Kohlinger, F., Greimel, R., Afonso, A., Parker, Q. A., Kong, A. K. H., Bassa, C., Pleunis, Z.
Publikováno v:
A&A 609, A105 (2018)
One-opposition near-Earth asteroids (NEAs) are growing in number, and they must be recovered to prevent loss and mismatch risk, and to improve their orbits, as they are likely to be too faint for detection in shallow surveys at future apparitions. We
Externí odkaz:
http://arxiv.org/abs/1711.00709
Autor:
Casamiquela, L., Carrera, R., Blanco-Cuaresma, S., Jordi, C., Balaguer-Núñez, L., Pancino, E., Anders, F., Chiappini, C., Díaz-Pérez, L., Aguado, D. S., Aparicio, A., Garcia-Dias, R., Heiter, U., Martínez-Vázquez, C. E., Murabito, S., del Pino, A.
Open Clusters have long been used to study the chemo-dynamical evolution of the Galactic disk. This requires an homogeneously analysed sample covering a wide range of ages and distances. In this aper we present the OCCASO second data release. This co
Externí odkaz:
http://arxiv.org/abs/1706.03656
Autor:
Casamiquela, L., Carrera, R., Jordi, C., Balaguer-Núñez, L., Pancino, E., Hidalgo, S. L., Martínez-Vázquez, C. E., Murabito, S., del Pino, A., Aparicio, A., Blanco-Cuaresma, S., Gallart, C.
Open clusters (OCs) are crucial for studying the formation and evolution of the Galactic disc. However, the lack of a large number of OCs analyzed homogeneously hampers the investigations about chemical patterns and the existence of Galactocentric ra
Externí odkaz:
http://arxiv.org/abs/1603.00659
Autor:
Damasso, M., Esposito, M., Nascimbeni, V., Desidera, S., Bonomo, A. S., Bieryla, A., Malavolta, L., Biazzo, K., Sozzetti, A., Covino, E., Latham, D. W., Gandolfi, D., Rainer, M., Petrovich, C., Collins, K. A., Boccato, C., Claudi, R. U., Cosentino, R., Gratton, R., Lanza, A. F., Maggio, A., Micela, G., Molinari, E., Pagano, I., Piotto, G., Poretti, E., Smareglia, R., Di Fabrizio, L., Giacobbe, P., Gomez-Jimenez, M., Murabito, S., Molinaro, M., Affer, L., Barbieri, M., Bedin, L. R., Benatti, S., Borsa, F., Maldonado, J., Mancini, L., Scandariato, G., Southworth, J., Sanchez, R. Zanmar
Publikováno v:
A&A 581, L6 (2015)
Aims. For more than 1.5 years we monitored spectroscopically the star KELT-6 (BD+312447), known to host the transiting hot Saturn KELT-6b, because a previously observed long-term trend in radial velocity time series suggested the existence of an oute
Externí odkaz:
http://arxiv.org/abs/1508.06520
Autor:
Mancini, L., Esposito, M., Covino, E., Raia, G., Southworth, J., Tregloan-Reed, J., Biazzo, K., Bonomo, A., Desidera, S., Lanza, A. F., Maciejewski, G., Poretti, E., Sozzetti, A., Borsa, F., Bruni, I., Ciceri, S., Claudi, R., Cosentino, R., Gratton, R., Fiorenzano, A. F. Martinez, Lodato, G., Lorenzi, V., Marzari, F., Murabito, S., Affer, L., Bignamini, A., Bedin, L. R., Boccato, C., Damasso, M., Henning, Th., Maggio, A., Micela, G., Molinari, E., Pagano, I., Piotto, G., Rainer, M., Scandariato, G., Smareglia, R., Sanchez, R. Zanmar
Publikováno v:
Astronomy & Astrophysics 579, A136, 2015
We determine the true and the projected obliquity of HAT-P-36 and WASP-11/HAT-P-10 systems, respectively, which are both composed of a relatively cool star and a hot-Jupiter planet. Thanks to the high-resolution spectrograph HARPS-N, we observed the
Externí odkaz:
http://arxiv.org/abs/1503.01787
Autor:
Damasso, M., Biazzo, K., Bonomo, A. S., Desidera, S., Lanza, A. F., Nascimbeni, V., Esposito, M., Scandariato, G., Sozzetti, A., Cosentino, R., Gratton, R., Malavolta, L., Rainer, M., Gandolfi, D., Poretti, E., Sanchez, R. Zanmar, Ribas, I., Santos, N., Affer, L., Andreuzzi, G., Barbieri, M., Bedin, L. R., Benatti, S., Bernagozzi, A., Bertolini, E., Bonavita, M., Borsa, F., Borsato, L., Boschin, W., Calcidese, P., Carbognani, A., Cenadelli, D., Christille, J. M., Claudi, R. U., Covino, E., Cunial, A., Giacobbe, P., Granata, V., Harutyunyan, A., Lattanzi, M. G., Leto, G., Libralato, M., Lodato, G., Lorenzi, V., Mancini, L., Fiorenzano, A. F. Martinez, Marzari, F., Masiero, S., Micela, G., Molinari, E., Molinaro, M., Munari, U., Murabito, S., Pagano, I., Pedani, M., Piotto, G., Rosenberg, A., Silvotti, R., Southworth, J.
Publikováno v:
A&A 575, A111 (2015)
XO-2 is the first confirmed wide stellar binary system where the almost twin components XO-2N and XO-2S have planets. This stimulated a detailed characterization study of the stellar and planetary components based on new observations. We collected hi
Externí odkaz:
http://arxiv.org/abs/1501.01424
Autor:
Carrera, R., Casamiquela, L., Balaguer-Núñez, L., Jordi, C., Pancino, E., Allende-Prieto, C., Blanco-Cuaresma, S., Mártinez-Vázquez, C. E., Murabito, S., del Pino, A., Aparicio, A., Gallart, C., Recio-Blanco, A.
We present the motivation, design and current status of the Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO). Using the high resolution spectroscopic facilities available at Spanish observatories, OCCASO will derive chemica
Externí odkaz:
http://arxiv.org/abs/1412.3509
Autor:
Monelli, M., Milone, A. P., Stetson, P. B., Marino, A. F., Cassisi, S., Molina, A. Del Pino, Salaris, M., Aparicio, A., Asplund, M., Grundahl, F., Piotto, G., Weiss, A., Carrera, R., Cebrian, M., Murabito, S., Pietrinferni, A., Sbordone, L.
We present a general overview and the first results of the SUMO project (a SUrvey of Multiple pOpulations in Globular Clusters). The objective of this survey is the study of multiple stellar populations in the largest sample of globular clusters homo
Externí odkaz:
http://arxiv.org/abs/1303.5187
Autor:
Nascimbeni, V., Cunial, A., Murabito, S., Sada, P. V., Aparicio, A., Piotto, G., Bedin, L. R., Milone, A. P., Rosenberg, A., Borsato, L., Damasso, M., Granata, V., Malavolta, L.
The TASTE project is searching for low-mass planets with the Transit Timing Variation (TTV) technique, by gathering high-precision, short-cadence light curves for a selected sample of transiting exoplanets. It has been claimed that the "hot Jupiter"
Externí odkaz:
http://arxiv.org/abs/1210.3045
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