Zobrazeno 1 - 10
of 44
pro vyhledávání: '"M. Buttu"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
B. Lomberg, S. N. Mellon, F. X. Schmider, L. Abe, Djamel Mékarnia, A. Agabi, Nicolas Crouzet, Y. de Pra, G. J. J. Talens, I. Laginja, M. Buttu, Michael J. Ireland, Eric E. Mamajek, E. J. W. de Mooij, M. Nowak, John I. Bailey, Remko Stuik, Ji Wang, Sylvestre Lacour, A.-M. Lagrange, S. R. Crawford, Rainer Kuschnig, L. Wang, Philippe Stee, Z. Hui, Ignas Snellen, Grant M. Kennedy, P. A. Strøm, A. Lecavelier des Etangs, Rudi B. Kuhn, Konstanze Zwintz, Matthew A. Kenworthy, Tristan Guillot, Patrick Dorval, Kevin B. Stevenson, Paul Kalas
Publikováno v:
Astronomy and Astrophysics, 648
Photometric monitoring of Beta Pictoris in 1981 showed anomalous fluctuations of up to 4% over several days, consistent with foreground material transiting the stellar disk. The subsequent discovery of the gas giant planet Beta Pictoris b and the pre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c28a5d11887507016ba7f1ae210f2498
http://hdl.handle.net/11390/1205975
http://hdl.handle.net/11390/1205975
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
E. Carretti, G. Aresu, M. Bachetti, M. Bartolini, F. Buffa, M. Burgay, M. Buttu, T. Caria, P. Castangia, S. Casu, R. Concu, A. Corongiu, G. L. Deiana, E. Egron, A. Fara, F. Gaudiomonte, V. Gusai, N. Iacolina, A. Ladu, S. Loru, P. Marongiu, A. Melis, P. Melis, C. Migoni, S. Milia, A. Navarrini, A. Orlati, P. Ortu, S. Palmas, A. Pellizzoni, D. Perrodin, M. Pilia, T. Pisanu, S. Poppi, I. Porceddu, S. Righini, A. Saba, G. Serra, L. Serrau, G. Surcis, A. Tarchi, A. Trois, V. Vacca, G. Valente, G. P. Vargiu
Publikováno v:
2017 International Conference on Electromagnetics in Advanced Applications (ICEAA).
The Sardinia Radio Telescope (SRT) is a new 64-m across radio astronomical facility located in Sardinia, Italy, and operated by the National Institute for Astrophysics (INAF). It can operate on a broad frequency range −300 MHz to 115 GHz, and is eq
Autor:
G. Serra, G. Valente, Elise Egron, M. Buttu, Federica Govoni, Maura Pilia, I. Prandoni, F. T. Nasir, A. Orlati, Alessio Trois, Andrea Tarchi, A. Pellizzoni, Roberto Ricci, C. Stanghellini, Matteo Murgia, S. Casu, Valentina Vacca, Gianni Comoretto, M. N. Iacolina, F. Loi, N. D'Amico, A. Orfei, Delphine Perrodin, Sergio Poppi, Francesco Gaudiomonte, Tonino Pisanu, Paola Castangia, Pietro Bolli, Raimondo Concu, S. Loru, Marco Bartolini, Alessandro Corongiu, Andrea Melis, Caterina Tiburzi, A. Fara, Alessandro Ridolfi, S. Righini, Matteo Bachetti, Ettore Carretti, F. Massi, C. Migoni, M. Burgay, D. Guidetti, A. Zanichelli, Steven Tingay, I. Porceddu
Publikováno v:
NASA Astrophysics Data System
[Abridged] The Sardinia Radio Telescope (SRT) is the new 64-m dish operated by INAF (Italy). Its active surface will allow us to observe at frequencies of up to 116 GHz. At the moment, three receivers, one per focal position, have been installed and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5517c279ad1509929b3a92e9505f2196
http://hdl.handle.net/20.500.12386/27202
http://hdl.handle.net/20.500.12386/27202
Autor:
M. Buttu, Simona Righini, Paweł Wolak, S. Buttaccio, Andrea Orlati, T. M. Belloni, Victoria Grinberg, Emrah Kalemci, Raimondo Concu, Jörn Wilms, Andrea Melis, Marcin P. Gawronski, C. Stanghellini, Alessandro Navarrini, E. Egron, Jerome Rodriguez, Giuseppe Maccaferri, M. Marongiu, P. de Vicente, Carlo Migoni, Matteo Bachetti, G. P. Vargiu, Marcello Giroletti, M. Cadolle Bel, S. Loru, A. Pellizzoni, Jun Yang, Stephane Corbel, Sera Markoff, Katja Pottschmidt, P. Cassaro, Maura Pilia, Alessio Trois, Matteo Stagni, L. Barbas, Michael Lindqvist, M. N. Iacolina
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 471(3), 2703-2714. Oxford University Press
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 471 (3), pp.2703-2714. 〈10.1093/mnras/stx1730〉
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2017, 471 (3), pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
NASA Astrophysics Data System
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 471 (3), pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 471, pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
Mon.Not.Roy.Astron.Soc., 2017, 471 (3), pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 471 (3), pp.2703-2714. 〈10.1093/mnras/stx1730〉
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2017, 471 (3), pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
NASA Astrophysics Data System
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 471 (3), pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 471, pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
Mon.Not.Roy.Astron.Soc., 2017, 471 (3), pp.2703-2714. ⟨10.1093/mnras/stx1730⟩
In September 2016, the microquasar Cygnus X-3 underwent a giant radio flare, which was monitored for 6 days with the Medicina Radio Astronomical Station and the Sardinia Radio Telescope. Long observations were performed in order to follow the evoluti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9569919d4739f1f1c9db1026b4002ab5
Autor:
G. P. Vargiu, M. Marongiu, Francesco Gaudiomonte, Tonino Pisanu, Gian Luigi Deiana, F. Loi, Alessandro Navarrini, Delphine Perrodin, E. Urru, D. Simeone, V. Vacca, G. Serra, S. Loru, M. Buttu, Andrea Melis, M. Cardillo, Maura Pilia, A. Ladu, Alessio Trois, Franco Buffa, G. Valente, Raimondo Concu, Matteo Bachetti, A. Pellizzoni, Roberto Ricci, P. Marongiu, S. Mulas, E. Egron, A. Giuliani, Antonietta Fara, Sergio Poppi, G. Murtas, M. N. Iacolina, A. Saba, Simona Righini, Carlo Migoni
Observations of supernova remnants (SNRs) are a powerful tool for investigating the later stages of stellar evolution, the properties of the ambient interstellar medium, and the physics of particle acceleration and shocks. For a fraction of SNRs, mul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe166b92ab2db5fcb9f699471cc1a7d5
http://hdl.handle.net/20.500.12386/27300
http://hdl.handle.net/20.500.12386/27300
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
SPIE Proceedings.
The software maintenance typically requires 40-80% of the overall project costs, and this considerable variability mostly depends on the software internal quality: the more the software is designed and implemented to constantly welcome new changes, t