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Post Info TOPIC: Thirty-five radio telescope observation


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International Year of Astronomy 2009 Very Large Astrometry Session
The 24-hour observation period is set to:

* observation start: Wednesday November 18, 2009 @ 18:00:00 UT
* observation end: Thursday November 19, 2009 @ 18:00:00 UT

The observational network of the IYA09 session consists of 25 geodetic VLBI stations and the 10 VLBA stations.
Name Code Observatory name and location
AIRA Ai Aira, Kagoshima, Japan
BADARY Bd Badary Radioastronomical Observatory, Russia
BR-VLBA Br VLBA near Brewster, WA, USA
CHICHI10 Cc Chichijima, Ogasawara, Japan
CRIMEA Sm Simeiz VLBI Station, Crimean Astrophysical Observatory, Ukraine
DSS13 13 Goldstone (DSN), CA, USA
EFLSBERG Eb Radio Telescope Effelsberg, Germany
FD-VLBA Fd VLBA near Ft. Davis, TX, USA
HN-VLBA Hn VLBA near Han****, NH, USA
HOBART26 Ho Mt. Pleasant Observatory, Hobart, Tasmania, Australia
KASHIM34 Kb Kashima Space Research Center, Japan
KOKEE Kk Kokee Park Geophysical Observatory, Kauai, HI, USA
KP-VLBA Kp VLBA on Kitt Peak, AZ, USA
LA-VLBA La VLBA near Los Alamos, NM, USA
MATERA Ma Matera CGS VLBI Station, Italy
METSAHOV Mh Metsähovi Radio Observatory, Finland
MK-VLBA Mk VLBA on Mauna Kea, HI, USA
NL-VLBA Nl VLBA near North Liberty, IA, USA
NOTO Nt Noto VLBI Station, Italy
NYALES20 Ny Ny Alesund Geodetic Observatory, Spitsbergen, Norway
OHIGGINS Oh German Antarctic Receiving Station O'Higgins, Antarctica
ONSALA60 On Onsala Space Observatory, Sweden
OV-VLBA Ov VLBA in Owens Valley, CA, USA
PIETOWN Pt VLBA near Pie Town, NM, USA
SC-VLBA Sc VLBA on St. Croix, VI, USA
SESHAN25 Sh Sheshan VLBI Station, Shanghai, China
SINTOTU3 S3 Shintotsukawa, Hokkaido, Japan
SVETLOE Sv Svetloe Radio Astronomy Observatory, Russia
TIGOCONC Tc Transportable Integrated Geodetic Observatory (TIGO), Concepción, Chile
TSUKUB32 Ts Tsukuba VLBI Station, Japan
URUMQI Ur Nanshan VLBI Station, Urumqi, China
WESTFORD Wf Westford Antenna, Haystack Observatory, MA, USA
WETTZELL Wz Fundamentalstation Wettzell, Germany
YEBES40M Ys National Astronomical Observatory Yebes, Guadalajara, Spain
ZELENCHK Zc Radioastronomical Observatory Zelenchukskaya, Russia

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Thirty-five radio telescopes around the world will conduct an unprecedented continuous 24-hour observation of nearly 250 remote quasars this week. The collection of quasars, whose positions in the sky are precisely known, forms the core (or defining sources) of a grid of celestial landmarks called the International Celestial Reference Frame (ICRF2), which was officially recognised as the fundamental reference system for astronomy by the International Astronomical Union (IAU) in August 2009. The ICRF2 has 295 defining sources that are spread evenly over the sky and out of which 243 will be observed. The small number of stations in the Southern Hemisphere is the reason why some of the southern defining sources will not be observed. The observation, the largest of this type ever conducted in terms of both the number of participating telescopes and the number of quasars to be observed, will mark the kickoff for the use of this new system. The session is also organised as a specific event for the International Year of Astronomy (IYA2009) and is dedicated to reach out to the public and to promote science with open doors at the radio telescopes.
Telescopes in Asia, Australia, Europe, North America, South America, Antarctica, and in the Pacific will coordinate for the observation, forming a special network called a Very Long Baseline Interferometer (VLBI). Such a network has the spatial resolution of a radio telescope as large as the network, allowing one to pinpoint positions of quasars to unprecedented precision. The 35-element world-size radio telescope that was put together for the event will be unique in its ability to observe most of the ICRF2 quasars at once and to strengthen the ICRF2 grid.
The observation is coordinated by the International VLBI Service for Geodesy and Astrometry (IVS) and will take place from Wednesday 18 November, 18:00 UT to Thursday 19 November, 18:00 UT.

Source IYA2009


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