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The Westerbork Synthesis Radio Telescope (WSRT) is an aperture synthesis interferometer built on the site of the former World War II Nazi detention and transit camp Westerbork, north of the village of Westerbork, Midden-Drenthe, in the northeastern Netherlands.
Overview

The WRST comprises fourteen 25-metre radio telescopes deployed in a linear array arranged on a 2.7 kilometres (1.7 mi) East-West line, of which 10 are in a fixed equidistant position, 2 are nearby on a 300 m rail track, and 2 are located a kilometer eastwards on another 200 m rail track. It has a similar arrangement to other radio telescopes such as the One-Mile Telescope, Australia Telescope Compact Array and the Ryle Telescope. Its Equatorial mount is what sets it apart from most other radio telescopes, most of which have an Altazimuth mount. This makes it specifically useful for specific types of science, like polarized emission research as the detectors maintain a constant orientation on the sky during an observation. Ten of the telescopes are on fixed mountings while the remaining two dishes are movable along two rail tracks. The telescope was completed in 1970 and underwent a major upgrade between 1995 – 2000.[1]

The telescopes in the array can operate at several frequencies between 120 MHz and 8.3 GHz with an instantaneous bandwidth of 120 MHz and 8092-line spectral resolution.[2] The WSRT is often combined with other telescopes around the world to perform very-long-baseline interferometry (VLBI) observations, being part of the European VLBI Network.[3] The telescope is operated by ASTRON, the Netherlands Institute for Radio Astronomy.

WSRT performed a major upgrade in 2013 as part of the APERTIF (APERture Tile In Focus) project, where the current detectors are replaced with focal-plane arrays.[4] This will allow a 25x larger field of view and will be used for large scale surveys of the northern sky, bringing back focus on the Hydrogen line for which it was originally designed, but also large pulsar searches and other science. The Telescope has been out of operation since 2015 and is planned to be back in full operation in winter 2019.

The WSRT is also an International GNSS Service site.[5]

WSRT observed galaxies in the Spitzer Infrared Nearby Galaxies Survey at wavelengths of 18 cm and 22 cm.[6]

The WSRT site is also hosting one of the two experimental EMBRACE (Electronic MultiBeam Radio Astronomy ConcEpt) phased array telescopes, part of the Phase 2 of the Square Kilometre Array (SKA) project.[7]
References

"History of the WRST | ASTRON". astron.nl. ASTRON. Archived from the original on 12 April 2019. Retrieved 7 December 2020.
"WSRT GUIDE TO OBSERVATIONS". astron.nl. ASTRON. Archived from the original on 3 January 2015. Retrieved 7 December 2020.
Introduction to the EVN, European VLBI Network.
What is Apertif?, ASTRON.
IGS Station: wsrt, International GNSS Service.
Braun, R.; Oosterloo, T. A.; Morganti, R.; Klein, U.; Beck, R. (2007). "The Westerbork SINGS survey. I. Overview and image atlas". Astronomy and Astrophysics. 461 (2): 455. arXiv:astro-ph/0610114. Bibcode:2007A&A...461..455B. doi:10.1051/0004-6361:20066092.

"EMBRACE". ASTRON. Retrieved 2015-05-17.

External links

Media related to Westerbork Synthesis Radio Telescope at Wikimedia Commons

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Radio astronomy
Concepts

Units (watt and jansky) Radio telescope (Radio window) Astronomical interferometer (History) Very Long Baseline Interferometry (VLBI) Astronomical radio source

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People

Elizabeth Alexander John G. Bolton Edward George Bowen Ronald Bracewell Jocelyn Bell Burnell Arthur Covington Nan Dieter-Conklin Frank Drake Cyril Hazard Antony Hewish Sebastian von Hoerner Karl Guthe Jansky Kenneth Kellermann Frank J. Kerr John D. Kraus Bernard Lovell Jan Oort Joseph Lade Pawsey Ruby Payne-Scott Arno Penzias Grote Reber Martin Ryle Govind Swarup Gart Westerhout Paul Wild Robert Wilson

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