Mullard Radio Astronomy Observatory

Mullard Radio Astronomy Observatory
Named after	Mullard
Location	United Kingdom
Coordinates	52°10′03″N 0°01′57″E / 52.1674°N 0.0326°E
Telescopes	4C Array; Arcminute Microkelvin Imager; Cambridge Low Frequency Synthesis Telescope; Cambridge Optical Aperture Synthesis Telescope; Half-Mile Telescope; Interplanetary Scintillation Array; One-Mile Telescope; Ryle Telescope ;
	Location of Mullard Radio Astronomy Observatory
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The Mullard Radio Astronomy Observatory (MRAO) is located near Cambridge, UK and is home to a number of the largest and most advanced aperture synthesis radio telescopes in the world, including the One-Mile Telescope, 5-km Ryle Telescope, and the Arcminute Microkelvin Imager. It was founded by the University of Cambridge and is part of the Cambridge University, Cavendish Laboratories, Astrophysics Department.

History

Radio interferometry started in the mid-1940s on the outskirts of Cambridge, but with funding from the Science Research Council and a corporate donation of £100,000 from Mullard Limited, a leading commercial manufacturer of thermionic valves.

Construction of the Mullard Radio Astronomy Observatory commenced at Lords Bridge Air Ammunition Park,^[1] a few kilometres to the west of Cambridge.

The observatory was founded under Martin Ryle of the Radio-Astronomy Group of the Cavendish Laboratory, University of Cambridge and was opened by Sir Edward Victor Appleton on 25 July 1957. This group is now known as the Cavendish Astrophysics Group.

Location

The observatory is located a few miles south-west of Cambridge at Harlton on a former ordnance storage site, next to the disused Oxford-Cambridge Varsity railway line.

A portion of the track bed of the railway, running nearly east-west for several miles, was used to form the main part of the "5km" radio-telescope and the Cambridge Low Frequency Synthesis Telescope.

Telescopes

Telescope	Year built	Status
Arcminute Microkelvin Imager Large Array	2007	Active
Arcminute Microkelvin Imager Small Array	2004	Active
Very Small Array (moved to Tenerife in 1999)	1998	Active
Cosmic Anisotropy Telescope made first high-resolution maps of Cosmic Microwave Background fluctuations	1995	Decommissioned
Cambridge Optical Aperture Synthesis Telescope (COAST) first aperture synthesis at optical wavelengths	1993	Operated on clear nights
One receiver from the e-MERLIN array	1990	Active
Cambridge Low Frequency Synthesis Telescope (CLFST)	1980	Decommissioned
Ryle Telescope (formerly 5-Kilometre Telescope)	1971	Decommissioned (repurposed for AMI LA in 2006)
Half-Mile Telescope	1968	Decommissioned
Interplanetary Scintillation Array discovered first pulsar	1967	Decommissioned
One-Mile Telescope	1964	Decommissioned
4C Array, first telescope at the Cambridge's new observatory, used to make the 4C catalogue	1958	Decommissioned

Gallery

The following photographs (except for the last 2 items) were taken in June 2014:

Platform and Lecture Room formerly part of Lord's Bridge Railway Station
Arcminute Microkelvin Imager - Large Array (AMI-LA)
Arcminute Microkelvin Imager - Small Array (AMI-SA)
Stitched panorama of the Cosmic Anisotropy Telescope enclosure
Part of the Cambridge Optical Aperture Synthesis Telescope
The interior of the bunker of the Cambridge Optical Aperture Synthesis Telescope
The receiver from the e-MERLIN array
Surviving Yagi antennas of the Cambridge Low Frequency Synthesis Telescope
Two Half-Mile Telescopes
Remains of the Interplanetary Scintillation Array
One-Mile Telescope (left), two of the Half-Mile Telescope (centre) and the remains of the 4C Array (right)
Remains of the 4C Array, with One-Mile Telescope in the background
Mullard EL34 Power Pentode. Mullard produced up to 40% of thermionic valves used by Britain during 1939-1945 War
Mullard Radio Astronomy Observatory plaque