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Browsing by Author "Giroletti, M"

Browsing by Author "Giroletti, M"

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  • Ackermann, M; Ajello, M; Baldini, L; Ballet, J; Barbiellini, G; Bastieri, D; Becerra Gonzalez, J; Bellazzini, R; Bissaldi, E; Blandford, R. D; Bloom, E. D; Bonino, R; Bottacini, E; Bregeon, J; Bruel, P; Buehler, R; Buson, S; Cameron, R. A; Caragiulo, M; Caraveo, P. A; Cavazzut, E; Cecchi, C; Cheung, C. C; Chiang, J; Chiaro, G; Ciprini, S; Conrad, J; Costantin, D; Costanza, F; Cutini, S; D'Ammando, F; de Palma, F; Desiante, R; Digel, S. W; Di Lalla, N; Di Mauro, M; Di Venere, L; Domi­nguez, A; Drell, P. S; Favuzzi, C; Fegan, S. J; Ferrara, E. C; Finke, J; Focke, W. B; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gasparrini, D; Giglietto, N; Giordano, F; Giroletti, M; Green, D; Grenier, I. A; Guillemo, L; Guiriec, S; Hartmann, D. H; Hays, E; Marcotulli, L; Horan, D; Jogler, T; Johannesson, G; Johnson, A. S; Kuss, M; Mura, G. La; Larsson, S; Latronico, L; Li, J; Longo, F; Mazziotta, M. N; Loparco, F; Lovellette, M. N; Lubrano, P; Magill, J. D; Maldera, S; Manfreda, A; Michelson, P. F; Mirabal, N; Mitthumsiri, W; Mizuno, T; Monzani, M. E|; Morselli, A; Moskalenko, I. V; Negro, M; Rando, R; Nuss, E; Ohsugi, T; Ojha, R; Omodei, N; Orienti, M; Orlando, E; Ormes, J. F; Paliya, V. S; Paneque, D; Perkins, J. S; Rani, B; Persic, M; Pesce-Rollins, M; Piron, F; Porter, T. A; Principe, G; Raino, S; Razzano, M; Razzaque, S; Reimer, A; Reimer, O; Roman, R. W; Sgro, C; Simone, D; Siskind, E. J; Spada, F; Spandre, G; Spinelli, P; Stalin, C. S; 12 others (IOP Publishing, 2017-03-01)
    The detection of high-redshift ($z\,\gt 3$) blazars enables the study of the evolution of the most luminous relativistic jets over cosmic time. More importantly, high-redshift blazars tend to host massive black holes and ...
  • Paragi, Z; Godfrey, L; Reynolds, C; Rioja, M. J; Deller, A; Zhang, B; Gurvits, L; Bietenholz, M; Szomoru, A; Bignall, H. E; Boven, P; Charlot, P; Dodson, R; Frey, S; Garrett, M. A; Imai, H; Lobanov, A; Reid, M. J; Ros, E; Van Langevelde, H. J; Zensus, A. J; Zheng, X W; Alberdi, A; Agudo, I; An, T; Argo, M; Beswick, R; Biggs, A; Brunthaler, A; Campbell, B; Cimo, G; Colomer, F; Corbel, S; Conway, J. E; Cseh, D; Deane, R; Falcke, H .D. E; Gawronski, M; Gaylard, M; Giovannini, G; Giroletti, M; Goddi, C; Goedhart, S; Gomez, J. L; Gunn, A; Kharb, P; Kloeckner, H. R; Koerding, E; Kovalev, Y; Kunert-Bajraszewska, M; Lindqvist, M; Lister, M; Mantovani, F; Marti-Vidal, I; Mezcua, M; McKean, J; Middelberg, E; Miller-Jones, J. C. A; Moldon, J; Muxlow, T; O'Brien, T; Perez-Torres, M; Pogrebenko, S. V; Quick, J; Rushton, A; Schilizzi, R; Smirnov, O; Sohn, B .W; Surcis, G; Taylor, G. B; Tingay, S; Tudose, V. M; van der Horst, A; van Leeuwen, J; Venturi, T; Vermeulen, R; Vlemmings, W. H. T; de Witt, A; Wucknitz, O; Yang, J; Gabanyi, K; Jung, T (International School for Advanced Studies (SISSA), 2015-04)
    Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by providing phased-array outputs for SKA1-MID ...

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