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European VLBI Network information


European VLBI Network
The first e-VLBI science image produced by the European VLBI Network
Alternative namesEVN Edit this at Wikidata
Websitewww.evlbi.org Edit this at Wikidata
Telescopes
  • Cambridge MERLIN telescope
  • Medicina 32-m radio telescope
  • Metsahovi 14m radio telescope
  • Nanshan Radio Telescope
  • Noto 32-m radio telescope
  • Onsala Space Observatory 20 m telescope
  • Onsala Space Observatory 25 m telescope
  • Sheshan 25m radio telescope
  • Toruń RT4
  • Wettzell 20m radio telescope
  • Arecibo Telescope
  • Effelsberg 100-m Radio Telescope
  • Hartebeesthoek Radio Astronomy Observatory
  • Lovell Telescope
  • Madrid Deep Space Communications Complex
  • Mark II
  • Westerbork Synthesis Radio Telescope
  • Yebes Observatory RT40m Edit this on Wikidata
 European VLBI Network Related media on Commons

The European VLBI Network (EVN) is a network of radio telescopes located primarily in Europe and Asia, with additional antennas in South Africa and Puerto Rico, which performs very high angular resolution observations of cosmic radio sources using very-long-baseline interferometry (VLBI). The EVN is the most sensitive VLBI array in the world, and the only one capable of real-time observations. The Joint Institute for VLBI ERIC (JIVE) acts as the central organisation in the EVN, providing both scientific user support and a correlator facility. Very Long Baseline Interferometry (VLBI) achieves ultra-high angular resolution and is a multi-disciplinary technique used in astronomy, geodesy and astrometry.

The EVN operates an open-sky policy, allowing anyone to propose an observation using the network[1]

  1. ^ "Using the EVN | EVLBI". www.evlbi.org. Retrieved 2020-02-07.

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European VLBI Network

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Messier 82

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many other supernovae likely occurred in previous decades. The European VLBI Network studied a number of potential supernova remnants in the galaxy in...

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processing facility. This process is known as Very Long Baseline Interferometry (VLBI). Interferometry does increase the total signal collected, but its primary...

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of some individual sources in the field have been made with the European VLBI Network at 1.6 GHz with a higher resolution than the Hubble maps. An HDF...

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