Paper
3 July 2000 Science with VERA: VLBI exploration of radio astrometry
Mareki Honma, Noriyuki Kawaguchi, Tetsuo Sasao
Author Affiliations +
Abstract
VERA (VLBI Exploration of Radio Astrometry), being promoted by National Astronomical Observatory of Japan in collaboration with several Japanese universities, is a new VLBI array for phase referencing astrometry approved to start its construction in 2000. VERA, the first VLBI array dedicated to phase referencing VLBI, has a dual beam antenna system which enables us to observe a Galactic maser source and a nearby reference source simultaneously to remove the atmospheric fluctuation, and will measure positions of Galactic maser sources relative to reference sources (QSOs and radio galaxies) with 10 microarcsec level accuracy. With that accuracy, VERA will be able to determine parallaxes and proper motions of maser sources in the whole Galaxy. The major science targets of VERA will include 3D structure of the Galaxy and the distribution of dark matter, physics of outflow in star forming regions and stellar envelopes, precise calibration of the period-luminosity relation of Mira-type stars, and structure an evolution of QSOs and radio galaxies.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mareki Honma, Noriyuki Kawaguchi, and Tetsuo Sasao "Science with VERA: VLBI exploration of radio astrometry", Proc. SPIE 4015, Radio Telescopes, (3 July 2000); https://doi.org/10.1117/12.390461
Lens.org Logo
CITATIONS
Cited by 21 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Galactic astronomy

Stars

Antennas

Calibration

Receivers

Motion measurement

Distance measurement

RELATED CONTENT

Spitzer operations: scheduling the out years
Proceedings of SPIE (September 13 2012)
A CSO submillimeter active optics system
Proceedings of SPIE (June 27 2006)
Green Bank Telescope and the Millimeter Array
Proceedings of SPIE (July 31 1998)
The Atacama Large Millimeter Array (ALMA)
Proceedings of SPIE (February 04 2003)
Newcomb: a small astrometric interferometer
Proceedings of SPIE (June 26 1995)
The eSMA: description and first results
Proceedings of SPIE (July 10 2008)

Back to Top