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Astronomers simulate real-time telescope as big as the world to study peculiar active galaxy Using a perfectly orchestrated world-wide network of radio telescopes, astronomers have produced a high-resolution map of an Active Galactic Nucleus (AGN) belonging to an unknown class of gamma-ray sources. The unusual source and the groundbreaking technique used to produce the image are detailed in a letter published today in Astronomy & Astrophysics.
Astronomers in the Netherlands catch supernova, observe relativistic expansion Astronomers from JIVE and ASTRON have observed a supernova with peculiar radio emission. In a paper published in Nature, the team led by JIVE's Zsolt Paragi reports, for the first time ever, detection of a relativistic outflow in a Type Ic supernova, thus supporting the link with the even more energetic Gamma Ray Bursts.
e-EVN aids detection of "extremely prolific supernova factory" The electronic European VLBI Network (e-EVN) was critical in the detection of an "extremely prolific supernova factory" in the buried nucleus of a starburst galaxy last year. The results are published in Astronomy & Astrophysics.
"Naked-eye" gamma-ray burst aimed squarely at earth gamma-ray animation The jet from a powerful gamma-ray burst on March 19 that was bright enough for human eyes to see, despite the distance of 7.5 billion light years, was aimed almost directly at Earth. The burst was observed by satellites and observatories around the world, including ASTRON’s Westerbork Synthesis Radio Telescope. Results of the observation are published today in an article in Nature authored by an international team of 93 astronomers, including Dutch astronomers of the University of Amsterdam, ASTRON, the University of Leiden and the Joint Institute for VLBI in Europe (JIVE).
Dr. Huib Jan van Langevelde is the new director of JIVE Huib Jan van Langevelde (44) has been a member of the JIVE staff for 12 years, holding various positions. Recently he has managed various international projects related to astronomical user software and computing. His astronomical research focuses on the circumstellar matter around young and old stars, with an emphasis on astrophysical masers.
Huygens detected by GBT! As part of the VLBI tracking of the ESA's Huygens planetray probe, the R.C.Byrd Green Bank Telescope of the National Radio Astronomy Observatory equipped with the ESA/JIVE-supplied Mk5 recorder was the first to detect the Huygens' carrier signal at the frequency of 2040 MHz. The spectrum with resolution of 900 mHz is obtained with the JIVE's Huygens Software Correlator will be used for reconstruction of the vertical profile of the wind in Titan's atmosphere.
Radio astronomers prepare to track the Huygens Probe in the atmosphere of Titan When the Huygens Probe makes its plunge into the atmosphere of Saturn's moon Titan on 14 January 2005, a network of radio telescopes located in Australia, China, Japan and the USA connected to the Data Processing centre at the Joint Institute for VLBI in Europe (JIVE) will help international teams of scientists extract the maximum possible amount of irreplaceable information from a planetary mission unique in human history.
Further eVLBI Progress Jodrell Bank's new 2.5 Gb/s connection was used in an eVLBI test for the first time yesterday (20th Dec 2004). Real-time fringes to Jodrell were detected from Westerbork, at 128Mb/s, and from Torun at 256Mb/s. These are the highest real-time eVLBI data rates achieved in Europe so far, quadrupling the previous record. This fringe plot shows individual integrations, for one sub-band, on the Jodrell Bank-Torun baseline.
JIVE on Dutch radio Huib van Langevelde was recently interviewed by Dutch radio on the subject of eVLBI.
Astronomers demonstrate Global Internet Telescope European and US radio astronomers have demonstrated a new way of observing the Universe - through the Internet! Using cutting-edge technology, the researchers have managed to observe a distant star by using the world's research networks to create a giant virtual telescope. The process has allowed them to image the object with unprecedented detail, in real-time; something which only a few years ago would have been impossible. The star chosen for this remarkable demonstration, called IRC+10420, is one of the most unusual in the sky. Surrounded by clouds of dusty gas and emitting strongly in radio waves, the object is poised at the end of its life, heading toward a cataclysmic explosion known as a 'supernova'.