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Paragi, Z |
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dc.contributor.author |
Godfrey, L |
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Reynolds, C |
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Rioja, M. J |
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dc.contributor.author |
Deller, A |
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Zhang, B |
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Gurvits, L |
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Szomoru, A |
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Bignall, H. E |
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Charlot, P |
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Dodson, R |
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dc.contributor.author |
Frey, S |
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Ros, E |
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Van Langevelde, H. J |
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dc.contributor.author |
Zensus, A. J |
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dc.contributor.author |
Zheng, X W |
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dc.contributor.author |
Alberdi, A |
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Agudo, I |
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An, T |
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Middelberg, E |
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Miller-Jones, J. C. A |
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Moldon, J |
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Muxlow, T |
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O'Brien, T |
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Perez-Torres, M |
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Pogrebenko, S. V |
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dc.contributor.author |
Quick, J |
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Rushton, A |
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Schilizzi, R |
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dc.contributor.author |
Smirnov, O |
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dc.contributor.author |
Sohn, B .W |
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dc.contributor.author |
Surcis, G |
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Taylor, G. B |
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Tingay, S |
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Tudose, V. M |
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van der Horst, A |
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dc.contributor.author |
van Leeuwen, J |
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dc.contributor.author |
Venturi, T |
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dc.contributor.author |
Vermeulen, R |
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dc.contributor.author |
Vlemmings, W. H. T |
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dc.contributor.author |
de Witt, A |
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dc.contributor.author |
Wucknitz, O |
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dc.contributor.author |
Yang, J |
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dc.contributor.author |
Gabanyi, K |
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dc.contributor.author |
Jung, T |
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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 |