24–26 mars 2010
Epochal Tsukuba
Fuseau horaire Asia/Tokyo

Overview of VSOP-2(ASTRO-G) Project

Non programmé
Main Convention Hall (Epochal Tsukuba)

Main Convention Hall

Epochal Tsukuba

Tsukuba International Congress Center, 2-20-3,Takezono, Tsukuba,Ibaraki, 305-0032,Japan Tel: +81-29(861)0001 Fax: +81-29(861)1209

Orateur

Dr Tomofumi Umemoto (National Astronomical Observatory of Japan)

Description

Abstract: VSOP-2 (VLBI Space Observatory Progaramme 2) is a successor to VSOP/HALCA in which Japan plays a leading role. The space radio telescope (ASTRO-G) will be launched by Japan Aerospace Exploration Agency (JAXA) and will be operated as a single radio telescope with a 35,000km diameter, combined with grand radio telescopes. VSOP-2 will attain the angular resolution of about 40 micro-arcseconds at 43 GHz, 2,000 times better than the Hubble Space Telescope, and reveal the relativistic phenomena such as jets around super-massive black holes at the centers of galaxies, and the dynamics in galaxies and stars by observations of masers VSOP-2 project is now proceeding through the cooperation of the National Astronomical Observatory of Japan (NAOJ) and universities and institutes in Japan and all over the world, e.g., Europe, USA, Korea, China, Taiwan. NAOJ is expected to play vital roles in organizing the ground VLBI arrays and upgrading the ground facilities in the east-Asian region, East-Asian VLBI Network (EAVN), and construction and operation of science operation center to maximize science output.

Auteur principal

Dr Tomofumi Umemoto (National Astronomical Observatory of Japan)

Co-auteurs

Prof. Hideyuki Kobayashi (National Astronomical Observatory of Japan) Prof. Hirofumi Saito (JAXA) Prof. Masato Tsuboi (JAXA) Dr Yasuhiro Murata (JAXA) Dr Yoshiaki Hagiwara (National Astronomical Observatory of Japan)

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