Very long baseline interferometry with the SKA
dc.contributor.author | Paragi, Z. | |
dc.contributor.author | Godfrey, L. | |
dc.contributor.author | Reynolds, C. | |
dc.contributor.author | Rioja, M. | |
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. | |
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. | |
dc.contributor.author | Imai, H. | |
dc.contributor.author | Lobanov, A. | |
dc.contributor.author | Reid, M. | |
dc.contributor.author | Ros, E. | |
dc.contributor.author | Van Langevelde, H. | |
dc.contributor.author | Zensus, J. | |
dc.contributor.author | Zheng, X. | |
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, R. | |
dc.contributor.author | Cimó, G. | |
dc.contributor.author | Colomer, F. | |
dc.contributor.author | Corbel, S. | |
dc.contributor.author | Conway, J. | |
dc.contributor.author | Cseh, D. | |
dc.contributor.author | Deane, R. | |
dc.contributor.author | Falcke, H. | |
dc.contributor.author | Gabányi, K. | |
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 | Gómez, J. | |
dc.contributor.author | Gunn, A. | |
dc.contributor.author | Jung, T. | |
dc.contributor.author | Kharb, P. | |
dc.contributor.author | Klöckner, H. | |
dc.contributor.author | Körding, 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 | Martí-Vidal, I. | |
dc.contributor.author | Mezcua, M. | |
dc.contributor.author | Mckean, J. | |
dc.contributor.author | Middelberg, E. | |
dc.contributor.author | Miller-Jones, James | |
dc.contributor.author | Moldon, J. | |
dc.contributor.author | Muxlow, T. | |
dc.contributor.author | O'brien, T. | |
dc.contributor.author | Pérez-Torres, M. | |
dc.contributor.author | Pogrebenko, S. | |
dc.contributor.author | Quick, J. | |
dc.contributor.author | Rushton, A. | |
dc.contributor.author | Schilizzi, R. | |
dc.contributor.author | Smirno, O. | |
dc.contributor.author | Sohn, B. | |
dc.contributor.author | Surcis, G. | |
dc.contributor.author | Taylor, G. | |
dc.contributor.author | Tingay, S. | |
dc.contributor.author | Tudose, V. | |
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. | |
dc.contributor.author | De Witt, A. | |
dc.contributor.author | Wucknitz, O. | |
dc.contributor.author | Yang, J. | |
dc.date.accessioned | 2017-01-30T10:41:47Z | |
dc.date.available | 2017-01-30T10:41:47Z | |
dc.date.created | 2016-08-02T19:30:18Z | |
dc.date.issued | 2014 | |
dc.identifier.citation | Paragi, Z. and Godfrey, L. and Reynolds, C. and Rioja, M. and Deller, A. and Zhang, B. and Gurvits, L. et al. 2014. Very long baseline interferometry with the SKA. Proceedings of Science. (AASKA14) 143. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/4810 | |
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. | |
dc.publisher | SPIE - Internatioal Society for Optocal Engineering | |
dc.title | Very long baseline interferometry with the SKA | |
dc.type | Journal Article | |
dcterms.source.volume | 9-13-June-2014 | |
dcterms.source.title | Proceedings of Science | |
curtin.note |
This open access article is distributed under the Creative Commons license | |
curtin.department | Department of Physics and Astronomy | |
curtin.accessStatus | Open access |