| Name |
Location |
Remarks |
| Arcminute Microkelvin Imager |
Mullard Radio Astronomy Observatory, Cambridge, England |
|
| Dwingeloo (CAMRAS) |
Dwingeloo, Netherlands |
25 m steerable dish, formerly operated by ASTRON, now in restoration by CAMRAS [1] |
| Effelsberg |
Bad Münstereifel-Effelsberg near Bonn, Germany |
100 m dish operated by Max Planck Institut für Radioastronomie |
| European VLBI Network (EVN) |
Distributed across Europe with members located in China, South Africa and the USA |
VLBI array operated by the European Consortium for VLBI |
| IRAM - 30m |
Pico Veleta, in Granada, Spain |
30m dish operated by the Institute for Millimetric Radio Astronomy (Institut de Radio Astronomie Millimétrique, IRAM); works in the millimeter range (1mm to 3mm) both with superheterodyne and bolometric detectors. |
| Lovell Telescope |
Jodrell Bank Observatory, Cheshire, England |
76 m dish |
| RT-70(P-2500) |
Center for deep space communications, Evpatoria, Crimea, Ukraine |
RT-70, 70 m telescope, operating range 5–300 GHz |
| RT-70(P-2500) |
Galenki, Russia |
RT-70, 70 m telescope, operating range 5–300 GHz |
| RT-70(P-2500) |
plato Suffa, Uzbekistan |
RT-70, operating range 5–300 GHz |
| LOFAR (LOw Frequency ARray) |
Netherlands, Germany; in the future, Great Britain, France,Poland |
Low frequency array of dipole antennas at 1.3 to 30m wavelengths, with a strongly distributed signal processing system. The telescope beam is constructed in software from combinations of antenna signals. |
| Mark II |
Jodrell Bank Observatory, Cheshire, England |
25 m dish |
| MERLIN (Multi-Element Radio Linked Interferometer Network) |
United Kingdom |
Consists of the Cambridge 32 m at Mullard Radio Astronomy Observatory, Darnhall, Defford, Tabley (also known as Pickmere) and Knockin. Also includes the Lovell and Mark II telescopes at Jodrell Bank. |
| Metsähovi Radio Observatory |
Kylmälä, Kirkkonummi, Finland |
13.7 m dish, operates at 2 to 150 GHz, surface accuracy 0.1 mm (rms). |
| Nançay Radio Telescope (NRT) |
Nançay, France |
|
| Northern Cross |
Medicina Radio Observatory, Medicina, Bologna, Italy [2] |
32000 m² interferometer, cylindrical-paraboloid steerable over NS., 408 MHz, Beam=3' |
| Plateau de Bure Interferometer |
Plateau de Bure, Grenoble, France |
Originally an array of 3 antennas, since 2005 has 6 antennas, operating at millimeter wavelengths. |
| RATAN-600 |
Bolshoi Zelenchuk, Russia |
600 m dish, operates at 610 MHz to 30 GHz, world's largest diameter individual radio telescope |
| Ryle Telescope |
Mullard Radio Astronomy Observatory, Cambridge, England |
Eight 13 m dishes, and is currently used as one part of the Arcminute Microkelvin Imager. |
| TNA 1500 |
Kalyasin, Russia [3] |
64 m fully steerable dish, up to 5.86 GHz |
| TNA 1500 |
Medvezhji Ozera(Bear Lakes), Russia [4] |
64 m fully steerable dish, up to 5.86 GHz |
| Toruń RT4 32 m |
Toruń Centre for Astronomy, Toruń, Poland |
RT4 (32 m) parabolic antenna |
| Toruń RT3 15 m |
Toruń Centre for Astronomy, Toruń, Poland |
RT3 (15 m) antenna. |
| Ukrainian T-shaped Radio telescope, second modification (UTR-2) |
Grakovo, Kharkiv, Ukraine |
World's largest radio telescope at decametre wavelengths (max. collective area 150 000 m²). |
| Very Small Array (VSA) |
Observatorio del Teide, Canary Islands, Spain |
Array of 14 dishes, with two larger source-subtraction dishes. Controlled remotely from UK. |
| Westerbork Synthesis Radio Telescope (WSRT) |
Westerbork, Netherlands |
Array of radio telescopes [5] |
| Yebes RT 40 m |
Observatorio Astronómico Nacional, Yebes, Guadalajara, Spain [6] |
40 m parabolic steerable telescope for mm and cm wavelenghts |
| 32 m |
Ventspils International Radio Astronomy Center, Irbene, Latvia |
32-meter fully steerable parabolic, centimetre-wave range antenna RT-32 http://www.virac.lv/ |
| 32 m VLBI dish |
Medicina Radio Observatory, Medicina, Bologna, Italy [7] |
32 m, fully steerable dish, 1400 MHz...43 GHz |
| 32 m VLBI dish |
Noto Radio Observatory, Noto, Italy, [8] |
32 m, fully steerable dish, 300 MHz-86 GHz. Operates both as part of astronomical and geodetic VLBI network and as a single dish. |
| 25 m telescope |
Onsala Space Observatory, Onsala, Sweden |
25 m telescope |
| 22 m telescope |
Simeiz Observatory, Simeiz, Crimea, Ukraine |
22-m radio telescope for mm and cm radio waves. Located at the foot of mount Koshka (Cat) in Katsiveli (near Simeiz). Belongs to the Crimean Astrophysical Observatory, the Department of Radioastronomy. |
| 20 m telescope |
Onsala Space Observatory, Onsala, Sweden |
20 m telescope |
| ADU-1000 |
Center for deep space communications, Evpatoria, Crimea, Ukraine |
8 mirrors with diameter of 16 meters. Square is 1000 sq. meters. |
| 16 m |
Ventspils International Radio Astronomy Center, Irbene, Latvia |
16-meter diameter antenna RT-16 http://www.virac.lv/ |
| RT-7.5 (Bauman's radio telescope) |
Moscow Oblast, Russia |
Two 7.75-meter diameter antennas (only one is working at the moment) Remote access computer-aided laboratory |
| Name |
Location |
Remarks |
| Allen Telescope Array |
Hat Creek Radio Observatory, Hat Creek, California, USA |
42 6-m gregorian offset dishes using log periodic cooled feed covering .5GHz - 11.5GHz. Operated by joint agreement between Radio Astronomy Laboratory, University of California, Berkeley and the SETI Institute |
| Arecibo Observatory |
Arecibo, Puerto Rico |
World's largest single-dish radio telescope. |
| ARO 12m Radio Telescope |
Kitt Peak National Observatory, Tucson, Arizona, USA |
Previously operated by the NRAO, this telescope is currently operated by the University of Arizona's Arizona Radio Observatory, part of Steward Observatory. |
| Caltech Submillimeter Observatory |
Mauna Kea Observatory, Hawaii, USA |
10.4 m (34 ft) diameter submillimeter wavelength telescope |
| Combined Array for Research in Millimeter-wave Astronomy (CARMA) |
Owens Valley Radio Observatory, Big Pine, California, USA |
Heterogeneous interferometer array composed of 6 10-m elements, 9 6-m elements, covering frequencies ranging from 75-115GHz, ~230, and ~345GHz. Operated by joint agreements between Radio Astronomy Laboratory University of California, Berkeley, Caltech, University of Maryland, College Park, University of Illinois, Urbana-Champaign |
| Five College Radio Astronomy Observatory (FCRAO) |
Amherst, Massachusetts, USA |
Operated by UMass Amherst |
| Green Bank Interferometer (GBI) |
Green Bank, West Virginia, USA |
Three 26 meter (85 ft) radio telescopes operated by NRAO |
| Green Bank Telescope (GBT) |
Green Bank, West Virginia, USA |
World's largest fully mobile single-dish radio telescope |
| Heinrich Hertz Submillimeter Telescope (SMT) |
Mount Graham, Arizona, USA |
10-meter radio telescope operated by the University of Arizona's Arizona Radio Observatory, part of Steward Observatory. |
| James Clerk Maxwell Telescope |
Mauna Kea Observatory, Hawaii, USA |
15-metre submillimetre-wavelength telescope operated by the Joint Astronomy Centre |
| Large Millimeter Telescope (LMT) |
Sierra Negra, Puebla, Mexico |
A 50 m. telescope in millimetric wavelengths, the largest single dish instrument operating at this frequencies. |
| Morehead State University 21m. |
Morehead, Kentucky, USA |
A 21 m. telescope used for academic research and satellite data retrieval and control. |
| Solar monitor, two 1.8 m dishes |
Dominion Radio Astrophysical Observatory, Penticton, British Columbia, Canada |
The first dish here was originally a backup for the Algonquin site, but when the AGO site was later closed its instrument moved to DRAO and became its backup. |
| SRI International Antenna Facility |
Palo Alto, California, USA |
45.7 m parabolic reflector. Owned by the U.S. Government and constructed by SRI on land leased from Stanford University, the Antenna Facility is known locally as "the Dish." |
| Submillimeter Array (SMA) |
Mauna Kea Observatory, Hawaii, USA |
Operated jointly by the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics of Taiwan. |
| Synthesis Telescope, seven-element interferometer |
Dominion Radio Astrophysical Observatory, Penticton, British Columbia, Canada |
|
| Very Large Array (VLA) |
Socorro, New Mexico, USA |
Array of 27 dishes. Part of NRAO. |
| Very Long Baseline Array (VLBA) |
Socorro, New Mexico USA
(operations center) |
Array system of 10 radio telescopes; dishes are located at Mauna Kea, Hawaii, Owens Valley, California, Brewster, Washington, Kitt Peak, Arizona, Pie Town, New Mexico, Los Alamos, New Mexico, Fort Davis, Texas, North Liberty, Iowa, Hancock, New Hampshire, and St. Croix, U.S. Virgin Islands. |
| 46 metre dish |
Algonquin Radio Observatory, Algonquin Park, Ontario, Canada |
Most recently operated by Natural Resources Canada as a member of the International VLBI Service |
| 26-m single-dish |
Dominion Radio Astrophysical Observatory, Penticton, British Columbia, Canada |
Formerly a BMEWS AN/FPS-92 antenna, likely re-located from Fort Churchill. |
| Two 26 m dishes |
Pisgah Astronomical Research Institute (PARI), Rosman, North Carolina, USA |
|