Japanese VLBI Network

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dc.creatorDoi, Akihiro
dc.creatorFujisawa, Kenta
dc.creatorHarada, Keiichiro
dc.creatorNagayama, Takumi
dc.creatorSuematsu, Kousuke
dc.creatorSugiyama, Koichiro
dc.creatorHabe, Asao
dc.creatorHonma, Mareki
dc.creatorKawaguchi, Noriyuki
dc.creatorKobayashi, Hideyuki
dc.creatorKoyama, Yasuhiro
dc.creatorMurata, Yasuhiro
dc.creatorOmodaka, Toshihiro
dc.creatorSorai, Kazuo
dc.creatorSudou, Hiroshi
dc.creatorTakaba, Hiroshi
dc.creatorTakashima, Kazuhiro
dc.creatorWakamatsu, Ken-ichi
dc.date2006-12-19
dc.date.accessioned2026-07-07T10:36:43Z
dc.date.available2026-07-07T10:36:43Z
dc.descriptionWe present the basic features and the activities of Japanese VLBI network (JVN), a newly-established VLBI network with baselines ranging from 50 to 2560 km spreading across the Japanese islands, and capable of observing at 6.7, 8.4, and 22 GHz. We show a number of results of JVN observations: 8.4-GHz continuum images of a Giga-hertz Peaked Spectrum (GPS) source and radio-loud Narrow-Line Seyfert 1 galaxies (NLS1s), the spatial and velocity structures of water masers in NML Cygni as well as methanol masers in Cep A, and demonstrative observations with the bigradient phase referencing.
dc.description3 pages, 2 figures, to appear in the proceedings of the 8th EVN symposium held in Torun, Poland, September 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0612528
dc.identifierhttp://arxiv.org/abs/astro-ph/0612528
dc.identifierPoS8thEVN:071,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180148
dc.subjectAstrophysics
dc.titleJapanese VLBI Network
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