Very Long Baseline Interferometry with the SKA

Z Paragi,L Godfrey,Cormac Reynolds,Maria J Rioja,Adam T Deller,Bo Zhang,Leonid I Gurvits,Michael F Bietenholz,Arpad Szomoru,Hayley E Bignall, Paul Boven,Patrick Charlot,Richard G Dodson,Sandor Frey,M A Garrett,Hiroshi Imai,Andrei P Lobanov,Mark J Reid,E Ros,Huib Van Langevelde,J Anton Zensus,X W Zheng,Antxon Alberdi,Ivan Agudo,Tao An, M K Argo,R J Beswick, A D Biggs,A Brunthaler,R M Campbell,Giuseppe Cimo,Francisco Colomer,S Corbel,J Conway,D Cseh,R P Deane,H Falcke,K E Gabanyi,Marcin P Gawronski,Michael J Gaylard, G Giovannini, M Giroletti,C Goddi,Sharmila Goedhart,J L Gomez, Alastair Gunn,Taehyun Jung,P Kharb,H R Klockner, E Kording,Y Y Kovalev,M Kunertbajraszewska,M Lindqvist,M L Lister,F Mantovani,I Martividal,M Mezcua,J P Mckean,Enno Middelberg,J C A Millerjones,J Moldon,T W B Muxlow,Tim Obrien,M A Pereztorres,Sergei V Pogrebenko,Jonathan F H Quick,Anthony Rushton, Richard T N Schilizzi,O Smirnov,Bong Won Sohn,G Surcis,Greg Taylor,Steven J Tingay,V Tudose,Alexander Van Der Horst,Joeri Van Leeuwen,Tiziana Venturi, R C Vermeulen,W H T Vlemmings,Aletha De Witt,O Wucknitz,Jun Yang

Proceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14)（2015）

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摘要

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.

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