veraserver.mtk.nao.ac.jp

Toppage - VERA

Welcome to the VERA project. VERA (VLBI Exploration of Radio Astrometry) is a VLBI array to explore the 3-D structure of the Milky Way Galaxy based on high-precision astrometry of Galactic maser sources. Mizusawa VLBI Observatory invites applications for an assistant professor positon working on VLBI. List of accepted proposals for 2015A season is now available. Call-for-proposal of KaVA for 2015B. KaVA HP in KASI) 2015.04.15. Call-for-proposal of VERA for 2015B. National Astronomical Observatory of Japan.

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Toppage - VERA | veraserver.mtk.nao.ac.jp Reviews

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Welcome to the VERA project. VERA (VLBI Exploration of Radio Astrometry) is a VLBI array to explore the 3-D structure of the Milky Way Galaxy based on high-precision astrometry of Galactic maser sources. Mizusawa VLBI Observatory invites applications for an assistant professor positon working on VLBI. List of accepted proposals for 2015A season is now available. Call-for-proposal of KaVA for 2015B. KaVA HP in KASI) 2015.04.15. Call-for-proposal of VERA for 2015B. National Astronomical Observatory of Japan.

<META> KEYWORDS

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2 what's vera

3 system and stations

4 high light

5 common use

6 documents

7 japanese

8 sitemap

9 what's new

10 topics

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Toppage - VERA | veraserver.mtk.nao.ac.jp Reviews

https://veraserver.mtk.nao.ac.jp

Welcome to the VERA project. VERA (VLBI Exploration of Radio Astrometry) is a VLBI array to explore the 3-D structure of the Milky Way Galaxy based on high-precision astrometry of Galactic maser sources. Mizusawa VLBI Observatory invites applications for an assistant professor positon working on VLBI. List of accepted proposals for 2015A season is now available. Call-for-proposal of KaVA for 2015B. KaVA HP in KASI) 2015.04.15. Call-for-proposal of VERA for 2015B. National Astronomical Observatory of Japan.

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veraserver.mtk.nao.ac.jp

1

Hilight - VERA

http://veraserver.mtk.nao.ac.jp/hilight/index-e.html

First fringes have been successfully detected between KVN and VERA. First test observation has been made between KVN Yonsei station in Seoul and VERA Mizusawa station on 1st Nov. 2008, and fringes have been successfully detected at 22 GHz. KVN (Korean VLBI Network) is a new VLBI array that consists of three 21m-telescopes located in South Korea, and now KVN people have been working on the system evaluations to start its regular operation from 2009. Left: KVN Yonsei station in Seoul.

2

System & Stations - VERA

http://veraserver.mtk.nao.ac.jp/system/index-e.html

VERA array and stations. VERA array and stations. VERA array consists of 4 stations located at Mizusawa. National Astronomical Observatory of Japan. National Institutes of Natural Sciences. C) since 2000. All right reserved.

3

Common Use - VERA

http://veraserver.mtk.nao.ac.jp/restricted/CFP2015B.html

Call for Proposal of VERA -2015B-. Observing proposals for the VERA are invited for the observing period from August 15th 2015 to January 15th 2016. Deadline for proposal submission is. May 26th, 2015, 08:00 UT. In this observing period, following observing modes are available. Please refer to the VERA status reports. For more detail about each observing mode. Dual-beam mode : available for K-band and Q-band. Frequency band : K-band, Q-band and C-band (C-band is tentatively opened). Proposals must be rec...

4

Toppage - VERA

http://veraserver.mtk.nao.ac.jp/index.html

Welcome to the VERA project. VERA (VLBI Exploration of Radio Astrometry) is a VLBI array to explore the 3-D structure of the Milky Way Galaxy based on high-precision astrometry of Galactic maser sources. Call-for-proposal of KaVA for 2016B. Call-for-proposal of VERA for 2016B. List of accepted proposals for 2015B season is now available. Mizusawa VLBI Observatory invites applications for an assistant professor positon working on VLBI. First fringes have been successfully detected between KVN and VERA more.

5

トップページ－VERA

http://veraserver.mtk.nao.ac.jp/index-J.html

VERA "VLBI Exploration of Radio Astrometry VLBI技術. に日韓共同VLBI観測網本格運用開始うお座WX星周囲に見られる一酸化珪素メーザーの高画質２色撮像に成功. 鹿児島大学のRoss A. Burns氏を中心とした研究チームは、VERAを用いて大質量星形成領域S255の水メーザー観測を行い、S255領域でアウトフロー(物質の流出)、およびU字形のメーザー分布を検出しました。 C) since 2000. All right reserved.

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Toppage - VERA

Welcome to the VERA project. VERA (VLBI Exploration of Radio Astrometry) is a VLBI array to explore the 3-D structure of the Milky Way Galaxy based on high-precision astrometry of Galactic maser sources. Mizusawa VLBI Observatory invites applications for an assistant professor positon working on VLBI. List of accepted proposals for 2015A season is now available. Call-for-proposal of KaVA for 2015B. KaVA HP in KASI) 2015.04.15. Call-for-proposal of VERA for 2015B. National Astronomical Observatory of Japan.

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