PARAGI, Zsolt,; GODFREY, Leith,; REYNOLDS, Cormac,; RIOJA, Maria,; DELLER, Adam,; ZHANG, Bo,; GURVITS, Leonid,; BIETENHOLZ, Michael,; SZOMORU, Arpad,; BIGNALL, Hayley,; BOVEN, Paul,; CHARLOT, P.; DODSON, Richard,; FREY, Sandor,; GARRETT, Michael,; IMAI, Hiroshi,; LOBANOV, Andrei,; REID, Mark,; ROS, Eduardo,; VAN LANGEVELDE, Huib,; ZENSUS, J. Anton; ZHENG, Xing Wu,; ALBERDI, Antxon,; AGUDO, Ivan,; AN, Tao,; ARGO, Megan,; BESWICK, Rob,; BIGGS, Andy D.,; BRUNTHALER, Andreas,; CAMPBELL, Robert M.,; CIMO, Giuseppe,; COLOMER, Francisco,; CORBEL, Stephane,; CONWAY, John,; CSEH, David,; DEANE, Roger,; FALCKE, Heino,; GABANYI, Krisztina,; GAWRONSKI, Marcin,; GAYLARD, Michael,; GIOVANNINI, Gabriele,; GIROLETTI, Marcello,; GODDI, Ciriaco,; GOEDHART, Sharmila,; GOMEZ, Jose L.,; GUNN, Alastair,; JUNG, Taehyun,; KHARB, Preeti,; KLOCKNER, Hans-Rainer,; KORDING, Elmar,; KOVALEV, Yurii Yu.,; KUNERT-BAJRASZEWSKA, Magdalena,; LINDQVIST, Michael,; LISTER, Matt,; MANTOVANI, Franco,; MARTI-VIDAL, Ivan,; MEZCUA, Mar,; MCKEAN, John,; MIDDELBERG, Enno,; MILLER-JONES, James,; MOLDON, Javier,; MUXLOW, Tom,; O'BRIEN, Tim,; PÉREZ-TORRES, Miguel,; POGREBENKO, Sergei,; QUICK, Jonathan,; RUSHTON, Anthony P.,; SCHILIZZI, Richard,; SMIRNOV, Oleg,; SOHN, Bong Won,; SURCIS, Gabriele,; TAYLOR, Greg,; TINGAY, Steven,; TUDOSE, Valeriu,; VAN DER HORST, Alexander,; VAN LEEUWEN, Joeri,; VENTURI, Tiziana,; VERMEULEN, Rene,; VLEMMINGS, Wouter,; DE WITT, Aletha,; WUCKNITZ, Olaf,; YANG, Jun,

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Este ítem está publicado en

Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9 -13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.143, 2014-06-09, Giardini Naxos, Sicily. 2015p. id.143

Resumen en inglés

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.< Leer menos

Palabras clave en inglés

Astrophysics

Solar and Stellar Astrophysics

Astrophysics of Galaxies

Cosmology and Nongalactic Astrophysics

Instrumentation and Methods for Astrophysics

High Energy Astrophysical Phenomena

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804