Work

Japanese VLBI Network

Year: 2007

Type: conference-paper

Abstract: We present the basic features and the activities of Japanese VLBI network (JVN), a newlyestablished 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.

Source: European VLBI Network Symposium and Users Meeting (EVN Symposium)

DOI: 10.22323/1.036.0071

Authors: Akihiro Doi, Kenta Fujisawa, Keiichiro Harada, Takumi Nagayama, Kousuke Suematsu, Koichiro Sugiyama, Asao Habe, Mareki Honma, Noriyuki Kawaguchi, Hideyuki Kobayashi, Yasuhiro Koyama, Yasuhiro Murata, Toshihiro Omodaka, Kazuo Sorai, Hiroshi Sudo, Hiroshi Takaba, Kazuhiro Takashima, Ken-ichi Wakamatsu

Institutions: Yamaguchi University, Kagoshima University, Hokkaido University, National Astronomical Observatory of Japan, National Institute of Information and Communications Technology, Japan Aerospace Exploration Agency, Gifu University, Geospatial Information Authority of Japan

Language: English

Topic: Radio Astronomy Observations and Technology

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: hybrid

OpenAlex ID: W1669968637

FWCI: 2.324

Cites: 3

Cited by: 6

Related to: 10