The first purpose builtradiotelescopewent into operation in 1937.
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His 1937 radio antenna was the second ever to be used for astronomical purposes and the first parabolic reflecting antenna to be used as aradiotelescope.
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Britain has extensive experience of taking special measures to protect radio telescopes from harmful interference, under the oversight of a committee including representatives of the radioastronomy community.
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The cosmic microwave background radiation was also first detected using radio telescopes.
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Because radio telescopes have low resolution, they were the first instruments to use interferometry allowing two or more widely separated instruments to simultaneously observe the same source.
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Voyager 1 can not be seen in visible light, but its radio signal is very bright compared to most natural things studied by radio telescopes.
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Recent advances include greater emphasis on experiments at optical wavelengths, and the construction of a newradiotelescopethat is deliberately designed for such reconnaissance.
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The present capabilities of this technology allow a new type ofradiotelescopeto be built : an array of hundreds of small (and therefore, relatively inexpensive) antennas.
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It is probably the most powerfulradiotelescopein the world.
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Essentially, there are two types ofradiotelescope.
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This dictates the dish size aradiotelescopeneeds for a useful resolution.
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Currently, it consists of nine optical telescopes and aradiotelescope, which is currently taken out of service.
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In this radar astronomy procedure radio waves of known wavelength are emitted from aradiotelescopeaimed at an asteroid.
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A typical size of the single antenna of aradiotelescopeis 25 meters.
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Microwave transitions are measured in the laboratory and matched to emissions from the interstellar medium using aradiotelescope.
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