| dc.contributor.author | Paragi, Z | |
| dc.contributor.author | Godfrey, L | |
| dc.contributor.author | Reynolds, C | |
| dc.contributor.author | Rioja, M. J | |
| dc.contributor.author | Deller, A | |
| dc.contributor.author | Zhang, B | |
| dc.contributor.author | Gurvits, L | |
| dc.contributor.author | Bietenholz, M | |
| dc.contributor.author | Szomoru, A | |
| dc.contributor.author | Bignall, H. E | |
| dc.contributor.author | Boven, P | |
| dc.contributor.author | Charlot, P | |
| dc.contributor.author | Dodson, R | |
| dc.contributor.author | Frey, S | |
| dc.contributor.author | Garrett, M. A | |
| dc.contributor.author | Imai, H | |
| dc.contributor.author | Lobanov, A | |
| dc.contributor.author | Reid, M. J | |
| dc.contributor.author | Ros, E | |
| dc.contributor.author | Van Langevelde, H. J | |
| dc.contributor.author | Zensus, A. J | |
| dc.contributor.author | Zheng, X W | |
| dc.contributor.author | Alberdi, A | |
| dc.contributor.author | Agudo, I | |
| dc.contributor.author | An, T | |
| dc.contributor.author | Argo, M | |
| dc.contributor.author | Beswick, R | |
| dc.contributor.author | Biggs, A | |
| dc.contributor.author | Brunthaler, A | |
| dc.contributor.author | Campbell, B | |
| dc.contributor.author | Cimo, G | |
| dc.contributor.author | Colomer, F | |
| dc.contributor.author | Corbel, S | |
| dc.contributor.author | Conway, J. E | |
| dc.contributor.author | Cseh, D | |
| dc.contributor.author | Deane, R | |
| dc.contributor.author | Falcke, H .D. E | |
| dc.contributor.author | Gawronski, M | |
| dc.contributor.author | Gaylard, M | |
| dc.contributor.author | Giovannini, G | |
| dc.contributor.author | Giroletti, M | |
| dc.contributor.author | Goddi, C | |
| dc.contributor.author | Goedhart, S | |
| dc.contributor.author | Gomez, J. L | |
| dc.contributor.author | Gunn, A | |
| dc.contributor.author | Kharb, P | |
| dc.contributor.author | Kloeckner, H. R | |
| dc.contributor.author | Koerding, E | |
| dc.contributor.author | Kovalev, Y | |
| dc.contributor.author | Kunert-Bajraszewska, M | |
| dc.contributor.author | Lindqvist, M | |
| dc.contributor.author | Lister, M | |
| dc.contributor.author | Mantovani, F | |
| dc.contributor.author | Marti-Vidal, I | |
| dc.contributor.author | Mezcua, M | |
| dc.contributor.author | McKean, J | |
| dc.contributor.author | Middelberg, E | |
| dc.contributor.author | Miller-Jones, J. C. A | |
| dc.contributor.author | Moldon, J | |
| dc.contributor.author | Muxlow, T | |
| dc.contributor.author | O'Brien, T | |
| dc.contributor.author | Perez-Torres, M | |
| dc.contributor.author | Pogrebenko, S. V | |
| dc.contributor.author | Quick, J | |
| dc.contributor.author | Rushton, A | |
| dc.contributor.author | Schilizzi, R | |
| dc.contributor.author | Smirnov, O | |
| dc.contributor.author | Sohn, B .W | |
| dc.contributor.author | Surcis, G | |
| dc.contributor.author | Taylor, G. B | |
| dc.contributor.author | Tingay, S | |
| dc.contributor.author | Tudose, V. M | |
| dc.contributor.author | van der Horst, A | |
| dc.contributor.author | van Leeuwen, J | |
| dc.contributor.author | Venturi, T | |
| dc.contributor.author | Vermeulen, R | |
| dc.contributor.author | Vlemmings, W. H. T | |
| dc.contributor.author | de Witt, A | |
| dc.contributor.author | Wucknitz, O | |
| dc.contributor.author | Yang, J | |
| dc.contributor.author | Gabanyi, K | |
| dc.contributor.author | Jung, T | |
| dc.date.accessioned | 2020-11-19T14:06:23Z | |
| dc.date.available | 2020-11-19T14:06:23Z | |
| dc.date.issued | 2015-04 | |
| dc.identifier.citation | Proceedings of Science, 143 | en_US |
| dc.identifier.issn | 1824-8039 | |
| dc.identifier.uri | http://prints.iiap.res.in/handle/2248/7298 | |
| dc.description | Open Access © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-ShareAlike Licence https://pos.sissa.it/215/143/pdf | en_US |
| dc.description.abstract | 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 and SKA1-SUR and using these extremely sensitive stations with other radio telescopes, and in SKA2 by realising a distributed configuration providing baselines up to thousands of km, merging it with existing VLBI networks. The motivation for and the possible realization of SKA-VLBI is described in this paper. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | International School for Advanced Studies (SISSA) | en_US |
| dc.relation.ispartofseries | Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14); | |
| dc.subject | Astrophysics | en_US |
| dc.subject | Cosmology and Nongalactic Astrophysics | en_US |
| dc.subject | Astrophysics of Galaxies | en_US |
| dc.subject | High Energy Astrophysical Phenomena | en_US |
| dc.subject | Solar and Stellar Astrophysics | en_US |
| dc.title | Very long baseline interferometry with the SKA | en_US |
| dc.type | Article | en_US |