Knowledge (XXG)

List of radio telescopes

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Radio optical Telescope with 54 m Spherical Reflector Antenna and 2.6 m optical telescope on the same axis. One of the most sensitive and low noise antennas in the world. Operating during 1987-2010. Conserved from 2015. It is planned to revitalize it in 2020-2025 by the force of Armenian
1506:
DKR-1000 is the world largest telescope operating in the meter wavelength range. A wide-band radio telescope instrument consists of two parabolic cylinders 1 km long and 40 m width. One cylinder extend from east to west and the 2nd from north to south. DKR-1000 has a high sensitivity and
526:
CSRH is an interferometer under construction in China. The CSRH will consist of 100 telescopes covering 0.4–15 GHz. 40 telescopes of 4.5 m cover 400 MHz – 2 GHz and 60 telescopes of 2 m cover 2–15 GHz. CSRH will be one of the world's largest and most advanced imaging
4688:
station now installed and operational in Nancay. The LOFAR Super Station (LSS) will increase the number of high sensitivity long baselines, provide short baselines and an alternate core, and be a large standalone instrument. It will operate in the low frequency band of LOFAR (30–80 MHz) and
706:
The SSRT is a crossed interferometer, consisting of two arrays of 128x128 parabolic antennas 2.5 meters in diameter each, spaced equidistantly at 4.9 meters and oriented in the E-W and N-S directions. The SSRT is a special-purpose solar radio telescope designed for studying solar activity in the
3761:
38-element radio telescope interferometer working in the frequency range of 1.2–6.0 GHz. The final baseline will be 2.27 km in the East-West and 1.17 km in the South directions, respectively. This instrument will obtain radio images from the sun with a spatial resolution ≈4x6 arc
940:
TRAO was established in October 1986 with the 13.7 meter Radio Telescope. It opened the new era of the millimeter-wave radio astronomy in Korea as one of the main facilities of Korea Astronomy and Space science Institute (KASI). It is operated by Radio astronomy division in KASI.
4706:
The Lunar Crater Radio Telescope (LCRT) is a proposal by the NASA Institute for Advanced Concepts to create an ultra-long-wavelength (hereby wavelengths greater than 10 m – i.e., frequencies below 30 MHz) radio telescope inside a lunar crater on the far side of the Moon.
971:(Constructing), Republic of Korea. They have an identical design and are equipped with a quasi-optical system that allows simultaneous observations at 22, 43, 86, and 129 GHz. Since August in 2013, KVN Ulsan have started to operate 6.7 GHz in single-dish and VLBI modes. 4838: 4802: 3836:
Main antenna is a cross-polarized square array composed of 18,432 half-wavelength dipoles. Research areas: Stable equatorial ionosphere, ionospheric field aligned irregularities, the dynamics of the equatorial neutral atmosphere and meteor physics.
4878: 3029:
37 m radome-enclosed 90 GHz radar/radiotelescope; 9 m radar for space debris tracking, 46 m incoherent scatter radar, 26 m L-band deep space tracking radar, 18 m radiotelescope used for geodesy. Operated by the
2358:
Low frequency array of dipole antennas at 1.25 to 30m wavelengths (10–240 MHz), with a strongly distributed signal processing system. The telescope beam is constructed in software from combinations of antenna signals. Operated by
4616:
Planned world's largest fully steerable single-dish radio telescope with a diameter of 110 meters. Operates at 300 MHz to 117 GHz. Construction of the telescope is planned to start in 2013 and completed within 10 years.
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Four 22 m fully steerable radio telescopes. At the 1960s the centimeter and millimeter-wavelength RT-22s had a world record-breaking high angular resolution for individual radio telescopes. Operated by the
3162:. The first station (LWA1) is 50 miles west of Socorro, colocated with the VLA. The second station is at the Sevilleta National Wildlife Refuge 20 miles north of Socorro. Additional stations are planned. 2020:
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.
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array composed of 6 10-m elements, 9 6-m elements, and 8 3.5-m elements covering frequencies ranging from 27–36 GHz, 80–115 GHz, and 215–265 GHz. Operated by joint agreements between
4754: 3210:
A 2.3-meter satellite dish on a fully steerable, motorized azimuth-elevation mount with a low-noise amplifier and super-heterodyne receiver running SRT/VSRT (version 7.5). Currently inactive.
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BSA is a Large Phased Array comprising over 16,000 dipoles and covering an area of 7.2 hectares. The BSA has a world record sensitivity in the meter wavelength range. Operated by the
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Abdalla, E.; Ferreira, E. G. M.; Landim, R. G.; Costa, A. A.; Fornazier, K. S. F.; Abdalla, F. B.; Barosi, L.; Brito, F. A.; Queiroz, A. R.; Villela, T.; Wang, B. (2021-08-19).
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An 18-meter telescope under development since 2010 for use by educators in Colorado and others. Sponsored by the Deep Space Exploration Society of Boulder County, Colorado
1641: 5013: 527:
spectroscopy instruments. CSRH will be used to study coronal mass ejections. All of the 4.5m telescopes are assembled and the 2m telescopes will be assembled by 2013.
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Extension of SKA-Phase to approximately 2000 dishes. This array, if built, would be 50 times more sensitive and 10,000 times faster than any other radio telescope.
777: 3726:
telescope with a 20 m main semi-axis primary reflector and a 17.8 m main semi-axis secondary reflector with 28 receivers, dedicated mainly to the detection of the
6919: 2705: 2071: 5392:"National Astronomical Research Institute of Thailand (Public Organization) - Thai – German relation wafts as 40-meter Radio Telescope pinpointed in Chiang Mai" 1361:
Low-frequency radio telescope of new generation. Construction is in progress, separate 25-element subarrays are used for observations of Sun, Jupiter, pulsars.
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in the world. Structural issues led to the decision to dismantle the structure. Before this could be done the instrument platform collapsed in December 2020.
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10.4 m (34 ft) diameter submillimeter wavelength telescope, closed since 2015, due to be dismantled since 2019 to return the land to the natives.
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The first dish here was originally a backup for the Algonquin site, but later the ARO instrument was moved to DRAO and this antenna became its backup.
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Fixed 256 array of 16-element dual-polarisation antennas covering 70–300 MHz with approximately 30° field-of-view using electronic beam-forming
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The Cool Universe: Observing Cosmic Dawn, ASP Conference Series, Vol. 344, Proceedings of the conference held 4–8 October 2004 in Valparaiso, Chile
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PaST is planned to be an array of some ten-thousand log-periodic antennas spread over several square kilometers. Construction started in 2004.
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32 m, fully steerable dish, 300 MHz – 86 GHz. Operates both as part of astronomical and geodetic VLBI network and as a single dish.
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A 45 m single-dish short-millimetre telescope, and six 10 m telescopes of the Nobeyama Millimetre Array (NMA), both operated by the
395: 372: 96:
The first radio telescope was invented in 1932, when Karl Jansky at Bell Telephone Laboratories observed radiation coming from the Milky Way.
7261: 6983: 6416: 4577: 4329: 3031: 1528: 1508: 1487: 1259: 1223: 1184: 1062: 1006: 7237: 7131: 3899: 2807: 2661: 2162: 1938: 213: 7229: 3995: 2741: 2392: 2141: 1747: 366: 6361:"Phase and pattern calibration of the Jicamarca Radio Observatory radar using satellites" (Document). Royal Astronomical Society. 2014. 3106:
A 50-meter telescope for observations at millimetre wavelengths, the largest single dish instrument operating in this wavelength band.
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The Nancay radio astronomy observatory and associated laboratories are developing the concept of a "Super Station" for extending the
906: 6899: 6721: 6664: 5716:"The Pushchino Radio Astronomy Observatory of the P N Lebedev Physical Institute Astro Space Center: yesterday, today, and tomorrow" 4359: 4269: 2455: 2433: 2338: 1030: 816: 492: 65: 7460: 6829: 6731: 4845: 4777: 3974: 3925: 2337:
A Small Network of Radio Telescopes and Radio Spectrographs doing Amateur Radio Astronomy at a Very High standard coordinated by
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A scientific and educational charitable company currently constructing a Radio Observatory and Ground Station in Cambridgeshire
1797:
A scientific and educational charitable company currently constructing a Radio Observatory and Ground Station in Cambridgeshire
7335: 6953: 5039: 4388: 3948: 3879: 3848: 3773: 3666: 3639: 3600: 3574: 3543: 1913:, closed in 1993, now owned by NRW-Stiftung, reopened 2010 after restoration and operated by Förderverein Astropeiler Stockert 1342: 588: 256: 7316: 7053: 6889: 3683: 3594: 3482: 3220: 2774: 2683: 2644: 2223: 1661: 883: 694: 652: 58: 6336: 2367: 2113: 30: 6524: 6739: 6603: 4865: 4287: 3968: 3633: 1921: 1618: 824: 726: 121: 7607: 6103: 93:
arrays. The list is sorted by region, then by name; unnamed telescopes are in reverse size order at the end of the list.
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seconds. Located in Cachoeira Paulista, São Paulo, Brazil (Latitude 45° 00' 20" West and Longitude 22° 41' 19" South)
3568: 3560: 3400: 3136: 2606: 2580: 2547: 2346: 2216: 1980: 752: 458: 381: 90: 7245: 5673: 2837:
Array of three 16-element dual-polarization tiles with electronic beam-forming. Identical to the original MWA design
2237:
Originally an array of 3 antennas, since 2005 has 6 antennas, operating at millimeter wavelengths, now part of NOEMA
5090: 7594: 6755: 5750: 5316: 4604: 3739: 3250: 3088: 3072: 2961: 2796: 2728:
5 m focal length cylinders, with an array of 256 dual-polarized radio receivers along the focus. Will map the
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A small radio telescope which, along with a twin instrument in Chile, has been continuously mapping interstellar
2715: 2668: 2261: 1868: 1771: 1507:
the telescope allows simultaneous observations at any wavelengths in the range from 2.5m to 10m. Operated by the
1217: 1025:. It is made up of 36 identical antennas, each 12 metres in diameter, with a 30 sq degrees FoV at 1.4 GHz. 5354: 4021: 7584: 7253: 7221: 7121: 6797: 6596: 3767: 3450: 3425: 3155: 2750: 2491: 2475: 2029: 1963: 1891: 1873: 1856: 1371: 1152: 466: 404: 2304: 1429:
600 m dish, operates at 610 MHz to 30 GHz, world's largest diameter individual radio telescope
6229: 5104: 792:
500m radio telescope, the world's largest filled-aperture radio telescope, operating range 70–3000 MHz.
7493: 7483: 6947: 6813: 5715: 3990:
antenna, with a focal array (4 beams @ 212 GHz, 2 beams @ 405 GHz) of room temperature receivers.
3625: 3215: 3017: 2639: 2529: 2282: 1602: 1589: 1104: 408: 5379: 7205: 7091: 5467: 4712: 4622: 4375: 4350: 4306: 4158: 3509:
Two 26m telescopes: 26 West and East. One 12m telescope, fully automated and accessed via PARI"s website.
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Netherlands, Germany, Great Britain, France, Sweden, Poland, Ireland; in future possibly other countries
248:
In progress – currently eight 6 m dishes with dual-polarization dipole antennas as feed at HartRAO.
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0.29-2.6 GHz; 2.95-7.8 GHz; 8–10 GHz; 12-15.4 GHz; 18–47 GHz; 67–100 GHz.
2815: 2665: 2610: 2601: 2480: 2204: 2199:
7.5 meter diameter antenna. Observable frequency range : 1.4–1.7 GHz. Bandwidth ≈9.2 MHz
1037: 898: 797: 325: 301: 282: 239: 219: 150: 5035: 3798: 2450: 2428: 2627:
dishes using log periodic cooled feed covering 0.5–11.5 GHz. Operated by joint agreement between
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A 30m aperture sub-millimeter telescope (TSMT) with an active reflector has been proposed in China.
3616:
54 dishes with 12-m diameter and 12 dishes with 7 m diameter, sensitive to wavelengths between
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30 m × 50 m, 768-element phased array and a 34 m diameter, 48-element phased array
7657: 7645: 7519: 7488: 7435: 7395: 7365: 7308: 7073: 6852: 6294: 6266: 6099: 5491: 5014:"This year will see major advances in South Africa and in international radio astronomy projects" 4402:
24-element aperture synthesis open source all-sky radio telescope, designed and developed by the
3820: 3745: 3172: 2005: 1906: 1243: 1054: 838:
Construction work started in 2017. A 40m single-dish short-millimetre telescope, operated by the
6174: 3705: 6578: 647:. It operates at a frequency of 326.5 MHz with a maximum bandwidth of 15 MHz at the front end. 7544: 7390: 6713: 6286: 5768: 5692: 5483: 5334: 4809: 4183: 3699: 3470: 3320: 2857: 2628: 2624: 2596:
46 metre fully steerable dish operated by Thoth Technology, Canada's largest radio telescope.
2310: 2288: 2267: 1631: 1227: 1163: 1010: 676: 644: 86: 6255:"The BINGO project. I. Baryon acoustic oscillations from integrated neutral gas observations" 2980:
43 m equatorial mount single-dish radio telescope. Currently awaiting its next mission.
2700:
6.1 metre dish with polarimeter back end. This telescope was decommissioned in April 2015.
2118: 1819: 1802: 7621: 7534: 7430: 7425: 7360: 7111: 6763: 6276: 5475: 4793: 4366: 4152: 3788:
13 dishes with 1 m diameter located at the Chajnantor plateau. Decommissioned in 2008.
3686:, and features an AzTEC millimeter camera in the focal plane of the dish, consisting of 144 3370: 3184:
A 21 m. telescope used for academic research and satellite data retrieval and control.
3083:
Single 14-meter reflector used for testing of the main HERA telescope. (Under Construction)
2326: 2190: 2046: 1767: 1366: 923:
telescope, consists of three rotatable cylindrical antennas (140 metres by 40 metres each).
888: 867: 228:
In progress – currently nineteen 14 m reflectors with crossed dipole antennas as feed.
3559:
60 cm telescope located on Cerro Toco and designed to measure the polarization of the
7455: 7400: 6644: 6619: 4930: 3864:
Array of telescopes located on Cerro Toco and designed to measure the polarization of the
3723: 3687: 2760: 2648: 2484: 1683:
32000 m² interferometer, cylindrical-paraboloid steerable over NS., 408 MHz, Beam=3'
1247: 1171: 1130: 1108: 1045: 871: 859: 640: 82: 6402: 4764:, Green Bank, West Virginia, US, the largest fully steerable radio telescope dish (2002) 7529: 7410: 6559: 4563: 4175: 4171: 4162: 4096: 4005: 3952: 3883: 3852: 3777: 3670: 3643: 3604: 3578: 3547: 3500: 3413: 3389: 3348: 3154:
A telescope composed of stations each with 256 crossed-dipole antennas operated by the
2792: 2632: 2584: 2546:
4.5 m single dish, and 115 m baseline 3 dish interferometer. Operated by the
2373: 2136: 2096: 1788: 1537: 1420: 1254:
64 m telescope (2nd largest movable dish in the Southern Hemisphere), operated by
911: 335: 6441: 5925:"NRW-Stiftung – Aktuelle News und Projekt der Woche: Schloss Harkotten im Munsterland" 1824: 334:
Now disassembled, PAPER at its maximum had 128 crossed dipole antennas, making it the
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World's largest 100-metre (330 ft) fully steerable single-dish radio telescope
2947: 2916: 2884: 2875: 2729: 2534: 2504: 2131:
13.7 m dish, operates at 2 to 150 GHz, surface accuracy 0.1 mm (rms).
1576: 1167: 4042:
35 m and 13.5 m Telescopes, Operated by Chinese Deep Space Network (CDSN)
2523:
However a 2019 video report shows that the place has been abandoned and scavenged.
7633: 7375: 6648: 4599:
12 m single dish, VLBI, in construction, expected to start operations in 2017
3682:
10 m telescope located at Pampa La Bola. This was a pathfinder instrument for
3404: 3094: 3044: 2459: 1775: 802: 657: 264: 192: 171: 6281: 5975:"Dwingeloo Radiotelescoop – CAMRAS – C.A. Muller Radioastronomie Station – PI9CAM" 5416: 4507: 3749: 2823: 2100: 53: 6340: 4479:
10 meter radio telescope in a highly elliptical earth orbit. Launched July 2011.
3937:
Full sun disk patrols with left- and right-hand circular polarization receivers.
7554: 7445: 7440: 7370: 6528: 4192: 4052: 2122: 1077: 968: 964: 598: 4634:
Additional 128 dishes merged with MeerKAT, expected to be operational in 2022.
3809:
13.7 m telescope, operates in the K and Q bands, with cryogenic receivers
6108: 5479: 3709: 3435: 3380: 3228: 3145: 3120: 2782: 2691: 2614: 2499: 2052: 1808: 1395: 863: 761: 630: 608: 6477: 6290: 6208: 6003: 5814:"Infraestructuras y trabajos de Astronomía del Instituto Geográfico Nacional" 5487: 5441:"China's new radio telescope will have dangerous solar eruptions in its gaze" 7559: 6787: 5577: 4591: 4521: 4237: 4100: 3691: 3458: 3446: 3167: 2396: 2145: 1985: 1860: 1834: 1519: 1498: 1477: 1415: 1334: 735: 5789:"Welcome to the site of one of the unique millimeter-range Radiotelescope!" 5788: 5627: 1018: 5950:"Astropeiler Stockert e.V. – Radioastronomie, Amateurfunk, Natur und mehr" 5677: 4989: 4200:
305 m (1,001 ft) Second largest single dish spherical reflector
57:
Four of the sixty four total antennas of the ALMA radio telescope, at the
7420: 7162: 5267:"Giant Metrewave Radio Telescope, Tata Institute of Fundamental Research" 4473: 3621: 3259: 3202:
Occidental College SRT (Small Radio Telescope), Hameetman Science Center
3176: 2828: 2733: 2463: 2415: 2248: 2229: 2210:
Distributed across Europe with members in China, South Africa and the US
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https://radio.kasi.re.kr/eavn/images/presentation/10.Kitiyane_Asanok.pdf
1656:
32-meter fully steerable parabolic, centimetre-wave range antenna RT-32
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12 antennas, operating at millimeter wavelengths (Operational: 2019).
7033: 6638: 5591: 5358: 5134: 4458: 4441: 4296: 3908: 3802: 3753: 3713: 3242: 3098: 2437: 2360: 2171: 2079: 2075: 2056: 2033: 2013: 2009: 1994: 1967: 1953: 1812: 1734: 1649: 1645: 1584:
Two 7.75-meter diameter antennas (only one is working at the moment)
1399: 1197: 643:
is a 530-metre (1,740 ft) long and 30-metre (98 ft) tall cylindrical
491:
L/C/S/X band receivers. 70 km south to Ürümqi. Operated by XAO (
260: 144: 5549: 5266: 4808:
The 530-metre (1,740 ft) long and 30-metre (98 ft) tall cylindrical
2410:
The European Radio Astronomy Club Telescope and Development Facility
1851:
30m dish operated by the Institute for Millimetric Radio Astronomy (
583:
Built in 2012. Operated by SHAO (Shanghai Astronomical Observatory)
7628: 7272:
Special Astrophysical Observatory of the Russian Academy of Science
6271: 5871: 5645: 5468:"MUSER and IPS telescopes for solar and space weather observations" 3700:
Baryon Acoustic Oscillations in Integrated Neutral Gas Observations
1021:, the Australian Square Kilometre Array Pathfinder, is operated by 666:
Operated by (Indian Institute of Astrophysics). A Radioheliograph.
403:
10-m microwave telescope making observations of clusters using the
7152: 6588: 6312: 5646:"CSIRO Parkes Observatory – Australia Telescope National Facility" 5563: 5535: 5112: 4869: 4849: 4587: 4434: 4009: 3956: 3942: 3887: 3856: 3781: 3674: 3647: 3617: 3608: 3582: 3551: 2736:
range of 0.8 to 2.5. Collected its first light in September 2017.
2725: 2091: 1610:
40 m parabolic steerable telescope for mm and cm wavelengths
1598: 1454: 1434: 1407: 1255: 1180: 1089: 1058: 1022: 960: 956: 769: 744: 721:
32 m RT-32 radio telescope, operating range 1.4–22 GHz.
277: 6372: 2153:
Eight 13 m dishes, and is currently used as one part of the
2063:
8 mirrors with diameter of 16 meters. Square is 1000 sq. meters.
1155:, approximately 1.6 km in length. Operates at 843 MHz. 6634: 5510:"China to start building giant telescope to monitor solar winds" 4383:
30 metre fully steerable dish operated by IRASR, AUT University
3417: 2925: 2924:
Three 26 meters (85 feet) radio telescopes formerly operated by
1897: 1720: 1296: 1093: 626: 594: 477:
25 m. Operated by SHAO (Shanghai Astronomical Observatory)
136: 6592: 6074: 5949: 4437:(Highly Advanced Laboratory for Communications and Astronomy) 3295:
Thirty-two crossed-dipole antennas measuring 100–200 MHz
2724:
A novel drift scan telescope, which consists of four 100 × 20
1855:, IRAM); works in the millimeter range (1mm to 3mm) both with 17: 6442:"Puerto Rico: Iconic Arecibo Observatory telescope collapses" 439: 6393:
Kohno, K. "The Atacama Submillimeter Telescope Experiment".
5043: 4305:
15-meter submillimetre-wavelength telescope operated by the
1564:
32m RT-32 radio telescope, operating range 1.4–22 GHz.
1548:
32m RT-32 radio telescope, operating range 1.4–22 GHz.
815:
Construction work started in 2012. Will be operated by XAO (
772:, the construction started in 1981 but was never completed. 6153: 5899: 5841: 3445:
Array system of 10 radio telescopes; dishes are located at
2856:
Synthesis telescope consists of seven 9-metre (30 ft)
2538: 6583: 6024: 3004: 2860:, three of which are movable along a 600-metre rail line. 2470:
Phased array and Digital back end based on the SKA design
2445:
Phased array and Digital back end based on the SKA design
457:
Dish diameter: 13.7 m. Site altitude: 3200 m. Operated by
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EAARO – East Anglian Astrophysiscal Research Organisation
607:
Thirty 45 m wire dishes; largest telescope at meter
6930:
Combined Array for Research in Millimeter-wave Astronomy
6128: 4559:
EAARO - East Anglian Astrophysical Research Organisation
4060:
35 m telescope and deep space antenna, operated by
3189:
Paul Plishner Radio Astronomy and Space Sciences Center
3000:
20m telescope, fully automated and accessed through the
2769:
Combined Array for Research in Millimeter-wave Astronomy
2341:
Research and Development Telescope in Mannheim Germany.
1708:
32 m, fully steerable dish, 1400 MHz...43 GHz
380:
13-element interferometer measuring anisotropies in the
4334:
Academia Sinica Institute of Astronomy and Astrophysics
3921:
Polarization Emission of Millimeter Activity at the Sun
3655:
12 m telescope located at the Chajnantor plateau.
3342:, the Antenna Facility is known locally as "The Dish." 1315:
Ukrainian T-shaped Radio telescope, second modification
71:
Ukrainian T-shaped Radio telescope, second modification
34: 2329:(Amateur Linked Long Baseline Interferometer Network) 1410:, 70 m telescope, operating range 5–300 GHz 955:
KVN consists of four 21-m radio telescopes located in
747:, 70 m telescope, operating range 5–300 GHz 7605: 5813: 5710: 5708: 3277:
Precision Array for Probing the Epoch of Reionization
320:
Precision Array for Probing the Epoch of Reionization
310:
Sixty four, 13.5 m dishes. A pathfinder for the
159:
7.6-metre (24.9 foot) dish with polarimeter back end
5536:"Korea Astronomy and Space science Institute (KASI)" 2404:
Small Array consists of 10 3.7-m parabolic antennas
1952:
2.8 km array of 14 25-meter dishes operated by
1737:(Multi-Element Radio Linked Interferometer Network) 1469:
64 m fully steerable dish, up to 5.86 GHz
1449:
64 m fully steerable dish, up to 5.86 GHz
1394:
former soviet Center for deep space communications,
840:
National Astronomical Research Institute of Thailand
234:
Hydrogen Intensity and Real-time Analysis eXperiment
81:– over one hundred – that are or have been used for 7512: 7474: 7328: 7293: 7180: 7145: 6872: 6694: 6679: 6626: 5160:"最新消息 – EurekAlert! 優睿科 – EurekAlert! Science News" 2747:
Center for Astrophysics | Harvard & Smithsonian
6230:"LMT – Large Millimeter Telescope Alfonso Serrano" 6049: 1088:1x70 m dish, 3x34 m dishes, operated by 858:A VLBI system with four 20-m telescopes in Japan ( 205:originally build as a technology demonstrator for 135:32-metre (104 foot) single dish, first of African 7034:Multi-Element Radio Linked Interferometer Network 4358:12 metre fully steerable dish operated by IRASR, 2831:Embry-Riddle Radio Observatory, Prescott AZ], US 2382:9.3 m solid surface dish, operated by PARAC 6525:"QTT International Advisory Workshop: About QTT" 6417:"Swedish-ESO 15m Submillimeter Telescope (SEST)" 5213:"Radio telescope under construction in Shanghai" 5185:"Large Radio Telescopes In China : Na Wang" 3694:pixels arranged in a compact hexagonal package. 3128:A 4.5-meter single dish, prototype dish for the 3077:Embry-Riddle Radio Observatory, Prescott AZ, US 338:with more elements than any other at that time. 6109:"URBEX | Epic abandoned Soviet radio telescope" 5894: 5892: 4746:Five hundred meter Aperture Spherical Telescope 4584:Alto Chorrillos, near San Antonio de los Cobres 1993:25 m steerable dish, formerly operated by 1337:wavelengths (max. collective area 150,000 m²). 907:Mingantu interplanetary scintillation telescope 778:Five hundred meter Aperture Spherical Telescope 6920:Canadian Hydrogen Intensity Mapping Experiment 6584:East Anglian Amateur Radio Observatory Website 5866: 5864: 5862: 5578:"Australian Square Kilometre Array Pathfinder" 5016:. Engineering News (Creamer Media). 2010-01-15 4463:Russian spacecraft carrying a radio telescope 3334:45.7 m parabolic reflector. Owned by the 2901:One of the most sensitive radars in the world 2706:Canadian Hydrogen Intensity Mapping Experiment 2664:, this telescope is currently operated by the 2072:Ventspils International Radio Astronomy Center 1642:Ventspils International Radio Astronomy Center 6604: 3894:4 m telescope located at Pampa La Bola. 3267:26m telescope built in 1958, operated by the 2521:and International science-technical society. 8: 6910:Australian Square Kilometre Array Pathfinder 6175:"Green Bank Observatory, 140 foot Telescope" 4016:15 m telescope. Decommissioned in 2003 1305:100 m fully steerable dish operated by 1000:Australian Square Kilometre Array Pathfinder 73:(UTR-2) radio telescope phased array antenna 6704:500 meter Aperture Spherical Telescope 5610:"Canberra Deep Space Communication Complex" 4830:Goldstone Deep Space Communications Complex 3338:and constructed by SRI on land leased from 3073:Hydrogen Epoch of Reionization Array (HERA) 6691: 6611: 6597: 6589: 6025:"ERAC – The European Radio Astronomy Club" 5668: 5666: 4816:near Ooty, Tamil Nadu, India (Early 1970s) 4796:, Jodrell Bank Observatory, England (1957) 4537:Under construction or planned construction 3661:Atacama Submillimeter Telescope Experiment 3589:6 m telescope located on Cerro Toco. 2732:of neutral hydrogen over the cosmological 2243:Northern Extended Millimeter Array (NOEMA) 1309:, operates at 395 MHz to 95 GHz 928:Taeduk Radio Astronomy Observatory (TRAO) 876:National Astronomical Observatory of Japan 687:National Astronomical Observatory of Japan 189:Hartebeesthoek Radio Astronomy Observatory 168:Hartebeesthoek Radio Astronomy Observatory 6280: 6270: 4886:Canberra Deep Space Communication Complex 3926:Complejo Astronomico El Leoncito (CASLEO) 3237:This cm wavelength telescope operated by 3056:10-meter radio telescope operated by the 1853:Institut de radioastronomie millimétrique 1147:Operated by the School of Physics at the 1071:Canberra Deep Space Communication Complex 517:Chinese Spectral Radio Heliograph (CSRH) 7024:Molonglo Observatory Synthesis Telescope 6861:Warkworth Radio Astronomical Observatory 6337:"Radio Observatorio do Itapetinga (ROI)" 5466:Yan, Yihua; et al. (8 March 2023). 4966: 4964: 4902:Madrid Deep Space Communications Complex 4748:(FAST), under construction, China (2016) 4689:extend this range to lower frequencies. 4644: 4540: 4416: 4251: 4214: 4134: 4073: 3986:1.5 m radome enclosed, single dish 3519: 3354:Dominion Radio Astrophysical Observatory 3304:Dominion Radio Astrophysical Observatory 2866:Five College Radio Astronomy Observatory 2843:Dominion Radio Astrophysical Observatory 2824:Distributed Array Radio Telescope (DART) 2712:Dominion Radio Astrophysical Observatory 2559: 1272: 1125:Molonglo Observatory Synthesis Telescope 981: 897:313 parabolic antennas for detection of 421: 348: 103: 64: 52: 7612: 6574:List of radio telescopes outside the US 5836: 5834: 5285:"Siberian Solar Radio Telescope (SSRT)" 4942: 4734: 2812:University of Illinois Urbana-Champaign 2423:From 14 kHz VLF up to 40 GHz 1911:Max Planck Institut für Radioastronomie 1746:Consists of the Cambridge 32 m at 1555:Svetloe Radio Astronomical Observatory 1307:Max Planck Institut für Radioastronomie 532:Miyun Synthesis Radio Telescope (MSRT) 6464: 6462: 5773:: CS1 maint: archived copy as title ( 5766: 5697:: CS1 maint: archived copy as title ( 5690: 5339:: CS1 maint: archived copy as title ( 5332: 4832:, Mojave Desert, California, US (1958) 4828:The 70 meter DSS 14 "Mars" antenna at 3843:Cosmology Large Angular Scale Surveyor 3491:Pisgah Astronomical Research Institute 3039:Heinrich Hertz Submillimeter Telescope 2829:https://erau-prescott-observatory.com/ 2051:Center for deep space communications, 1807:Center for deep space communications, 712:Badary Radio Astronomical Observatory 613:National Centre for Radio Astrophysics 272:5 meter (16 foot) parabolic reflector 7525:Cosmic microwave background radiation 7262:Pushchino Radio Astronomy Observatory 6984:Large Latin American Millimeter Array 5105:"Degree Angular Scale Interferometer" 4780:, in Bad Münstereifel, Germany (1971) 4578:Large Latin American Millimeter Array 4330:Smithsonian Astrophysical Observatory 4174:, with two larger source-subtraction 3300:Solar monitor, two 1.8 m dishes 3032:Massachusetts Institute of Technology 1529:Pushchino Radio Astronomy Observatory 1509:Pushchino Radio Astronomy Observatory 1488:Pushchino Radio Astronomy Observatory 1260:Australia Telescope National Facility 1224:Murchison Radio-astronomy Observatory 1209:26 m telescope, operated by the 1185:Australia Telescope National Facility 1116:30 m telescope, operated by the 1063:Australia Telescope National Facility 1007:Murchison Radio-astronomy Observatory 7: 7590: 7238:National Radio Astronomy Observatory 7132:Westerbork Synthesis Radio Telescope 4662:30m Sub-Millimeter Telescope (TSMT) 3900:Northeastern Space Radio Observatory 3192:Haswell, Kiowa County, Colorado, US 2808:University of Maryland, College Park 2163:Erciyes University Radio Observatory 1939:Westerbork Synthesis Radio Telescope 901:events. Operations started in 2023. 214:Hydrogen Epoch of Reionization Array 7230:Mullard Radio Astronomy Observatory 6470:"Radio telescopes – AUT University" 5592:"Australia Telescope Compact Array" 4900:The 70 meter DSS-63 antenna at the 4868:, Galenki, Russia, second of three 3996:Swedish-ESO Submillimetre Telescope 3963:Located at the Chajnantor plateau. 3506:327 MHz, 1.4 and 4.8 GHz 3347:Synthesis Telescope, seven-element 3271:. Currently undergoing renovation. 3245:monitoring program at 15 GHz. 2742:CfA 1.2 m Millimeter-Wave Telescope 2393:Mullard Radio Astronomy Observatory 2142:Mullard Radio Astronomy Observatory 1748:Mullard Radio Astronomy Observatory 1333:World's largest radio telescope at 367:Degree Angular Scale Interferometer 7064:Northern Extended Millimeter Array 6579:List of radio telescopes in the US 6527:. 24 December 2013. Archived from 6313:"Brazilian Decimetric Array (BDA)" 5550:"Radio astronomy division in KASI" 4921:List of astronomical observatories 4904:, near Madrid, Spain (late 1980s) 4872:in the former Soviet Union, (1984) 4852:in the former Soviet Union, (1978) 2977:0.75-15.0 GHz (2–40 cm) 2800:University of California, Berkeley 2476:64 m Sardinia Radio Telescope 291:Seven, 12 meter (39 foot) dishes. 14: 6900:Australia Telescope Compact Array 6722:Caltech Submillimeter Observatory 6665:Very Long Baseline Interferometry 4512:Chinese base on far side of Moon 4444:altitude of 21,400 km and a 4360:Auckland University of Technology 4270:Caltech Submillimeter Observatory 2456:The European Radio Astronomy Club 2434:The European Radio Astronomy Club 2339:The European Radio Astronomy Club 1896:Bad Münstereifel-Eschweiler near 1295:Bad Münstereifel-Effelsberg near 1031:Australia Telescope Compact Array 817:Xinjiang Astronomical Observatory 493:Xinjiang Astronomical Observatory 396:Amundsen–Scott South Pole Station 373:Amundsen–Scott South Pole Station 7663: 7651: 7639: 7627: 7615: 7589: 7580: 7579: 4893: 4877: 4857: 4837: 4821: 4801: 4785: 4769: 4753: 4737: 3975:Complejo Astronomico El Leoncito 3005:Skynet Robotic Telescope Network 2217:the European Consortium for VLBI 2086:16-meter diameter antenna RT-16 1390:Yevpatoria RT-70 radio telescope 1291:Effelsberg 100-m Radio Telescope 707:microwave range (5.7 GHz). 85:. The list includes both single 21: 6954:Giant Metrewave Radio Telescope 6822:UTR-2 decameter radio telescope 5357:. 16 March 2017. Archived from 5040:Durban University of Technology 4990:"HartRAO Radio Telescope Facts" 4884:The 70 meter DSS-43 antenna at 4389:Transient Array Radio Telescope 4178:. Controlled remotely from UK. 3949:Llano de Chajnantor Observatory 3880:Llano de Chajnantor Observatory 3849:Llano de Chajnantor Observatory 3774:Llano de Chajnantor Observatory 3667:Llano de Chajnantor Observatory 3640:Llano de Chajnantor Observatory 3601:Llano de Chajnantor Observatory 3575:Llano de Chajnantor Observatory 3544:Llano de Chajnantor Observatory 3418:The SETI League's Project Argus 3241:, is currently being used on a 1542:Karachaevo-Cherkessiya, Russia 1343:Giant Ukrainian Radio Telescope 589:Giant Metrewave Radio Telescope 257:Durban University of Technology 203:Experimental Demonstrator Model 7054:Northern Cross Radio Telescope 6890:Atacama Large Millimeter Array 3983:212 GHz and 405 GHz 3595:Atacama Large Millimeter Array 3483:St. Croix, U.S. Virgin Islands 3221:Owens Valley Radio Observatory 3168:Morehead State University 21m. 3002:University of North Carolina's 2896:Mojave Desert, California, US 2775:Owens Valley Radio Observatory 2684:Owens Valley Radio Observatory 2645:Kitt Peak National Observatory 2224:Plateau de Bure Interferometer 1662:Northern Cross Radio Telescope 1536:Radioastronomical Observatory 1193:Mount Pleasant Radio Telescope 1151:. East-west arm of the former 884:Daocheng Solar Radio Telescope 695:Siberian Solar Radio Telescope 653:Gauribidanur Radio Observatory 69:West arm of the low-frequency 59:Atacama Large Millimeter Array 1: 6373:"Jicamarca Radio Observatory" 5219:. 4 June 2015. Archived from 4288:James Clerk Maxwell Telescope 3969:Solar Submillimeter Telescope 3634:Atacama Pathfinder Experiment 2962:Green Bank 140 Foot Telescope 825:Thai National Radio Telescope 727:Galenki RT-70 radio telescope 7504:Gravitational-wave astronomy 7082:Primeval Structure Telescope 6259:Astronomy & Astrophysics 4888:, Canberra, Australia (1987) 4814:Ooty Radio Telescope Complex 4695:Lunar Crater Radio Telescope 3979:San Juan Province, Argentina 3930:San Juan Province, Argentina 3794:Itapetinga Radio Observatory 3728:Baryon Acoustic Oscillations 3205:Los Angeles, California, US 2388:Arcminute Microkelvin Imager 2155:Arcminute Microkelvin Imager 1595:Spanish National Observatory 1461:Medvezhji Ozera (Bear Lakes) 1179:22 m dish, operated by 1139:Australian Capital Territory 1082:Australian Capital Territory 921:interplanetary scintillation 574:Tian Ma 65m Radio Telescope 560:Kunming 40m Radio Telescope 541:Array of 28 9-meter dishes. 501:Primeval Structure Telescope 7416:Christiaan Alexander Muller 7282:Vermilion River Observatory 7190:Algonquin Radio Observatory 6655:Astronomical interferometer 6282:10.1051/0004-6361/202140883 5564:"Korean VLBI Network (KVN)" 5091:"PAPER a precursor to HERA" 4372:Warkworth Radio Observatory 4347:Warkworth Radio Observatory 3815:Jicamarca Radio Observatory 3569:Atacama Cosmology Telescope 3137:Long Wavelength Array (LWA) 2660:Previously operated by the 2607:Hat Creek Radio Observatory 2581:Algonquin Radio Observatory 2548:University of Hertfordshire 2114:Metsähovi Radio Observatory 1905:25 m dish operated by 1743:151 MHz – 24 GHz 1302:395 MHz – 95 GHz 753:Suffa RT-70 radio telescope 459:Purple Mountain Observatory 382:cosmic microwave background 7707: 6756:Large Millimeter Telescope 6075:"Radio Telescope Mannheim" 5472:Advances in Space Research 4778:Effelsberg Radio Telescope 4675:LOFAR Super Station (LSS) 4605:Qitai 110m Radio Telescope 4302:86, 230, and 345 GHz 4022:Estación de Espacio Lejano 3740:Brazilian Decimetric Array 3251:Peach Mountain Observatory 3089:Large Millimeter Telescope 2797:Radio Astronomy Laboratory 2577:Algonquin Radio Telescope 1922:Toruń Centre for Astronomy 1692:Medicina Radio Observatory 1667:Medicina Radio Observatory 1619:Toruń Centre for Astronomy 946:Korean VLBI Network (KVN) 835:300 MHz–115 GHz 812:300 MHz–117 GHz 672:Nobeyama radio observatory 546:Miyun 50m Radio Telescope 7575: 7044:Murchison Widefield Array 6964:Green Bank Interferometer 6788:RATAN-600 Radio Telescope 6671:Astronomical radio source 6129:"Home – Thoth Technology" 5480:10.1016/j.asr.2023.03.003 4916:Category:Radio telescopes 4848:, Crimea, first of three 4631:L-Band,X-Band,S-Band,UHF 4448:altitude of 560 km. 4342:Warkworth Radio Telescope 4233:Mauritius Radio Telescope 3358:Kaleden, British Columbia 3308:Kaleden, British Columbia 3160:Naval Research Laboratory 3061:Arizona Radio Observatory 2985:Green Bank 20m Telescope 2932:as a historic telescope. 2907:Green Bank Interferometer 2892:Goldstone Radio Telescope 2848:Kaleden, British Columbia 2716:Kaleden, British Columbia 2669:Arizona Radio Observatory 1997:, now operated by CAMRAS 1558:Svetloe, Karelia, Russia 1218:Murchison Widefield Array 1101:Ceduna Radio Observatory 855:6.7 GHz–43 GHz 715:Badary, Buryatia, Russia 700:Badary, Buryatia, Russia 132:3.8–6.4, 5, 6.7 GHz 7254:Onsala Space Observatory 7246:Nançay Radio Observatory 7222:Jodrell Bank Observatory 7122:Very Long Baseline Array 6798:Sardinia Radio Telescope 5514:South China Morning Post 5445:South China Morning Post 5217:Xinhua – English.news.cn 4718:Australia, South Africa 4628:Carnarvon, South Africa 4328:Operated jointly by the 3768:Cosmic Background Imager 3451:Owens Valley, California 3426:Very Long Baseline Array 3156:University of New Mexico 2751:Cambridge, Massachusetts 2492:Sardinia Radio Telescope 2368:São Gião radio telescope 2305:Nançay Radio Heliographe 2183:Wurzburg v2.0 LAB/OASU ( 2030:Onsala Space Observatory 1964:Onsala Space Observatory 1874:Jodrell Bank Observatory 1758:, Tabley (also known as 1372:Jodrell Bank Observatory 1153:Molonglo Cross Telescope 405:Sunyaev-Zeldovich effect 79:list of radio telescopes 7484:Submillimetre astronomy 7096:Australia, South Africa 6948:Event Horizon Telescope 4484:Ceased operations 2019 4468:Ceased operations 1966 4453:Ceased operations 2005 4116:Eiscat Radio Telescope 3626:submillimetre astronomy 3397:Very Small Array (VSA) 3216:OVRO 40 meter Telescope 3058:University of Arizona's 2666:University of Arizona's 2640:ARO 12m Radio Telescope 2530:Bayfordbury Observatory 2215:VLBI array operated by 1240:Parkes Radio Telescope 409:Event Horizon Telescope 407:. Also participates in 7206:Green Bank Observatory 7092:Square Kilometre Array 6209:"APEX instrumentation" 5632:Narrabri.atnf.csiro.au 5596:Narrabri.atnf.csiro.au 5135:"South Pole Telescope" 4713:Square Kilometer Array 4623:Square Kilometer Array 4526:Chinese lunar orbiter 4376:Warkworth, New Zealand 4351:Warkworth, New Zealand 4307:Joint Astronomy Centre 4159:Observatorio del Teide 4119:Adventdalen, Svalbard 3943:Q/U Imaging Experiment 3915:14.2 m telescope 3479:Hancock, New Hampshire 3467:Los Alamos, New Mexico 3269:University of Michigan 2349:(LOw Frequency ARray) 2283:Nançay Decameter Array 2262:Nançay Radio Telescope 1829:, 32 m telescope 1717:Noto Radio Observatory 1211:University of Tasmania 1160:Mopra Radio Telescope 1118:University of Tasmania 952:22/43/86/129 GHz 520:Inner Mongolia, China 312:Square Kilometre Array 74: 62: 7499:High-energy astronomy 7386:Sebastian von Hoerner 6994:Long Wavelength Array 6940:European VLBI Network 6880:Allen Telescope Array 6780:Qitai Radio Telescope 5271:Gmrt.ncra.tife.res.in 5247:Gmrt.ncra.tifr.res.in 4731:Gallery of big dishes 4320:Mauna Kea Observatory 4293:Mauna Kea Observatory 4275:Mauna Kea Observatory 3716:(under construction) 3538:Atacama B-Mode Search 3130:Allen Telescope Array 3112:Leuschner Observatory 2816:University of Chicago 2602:Allen Telescope Array 2205:European VLBI Network 1258:as part of the ATNF ( 1183:as part of the ATNF ( 1061:as part of the ATNF ( 1038:Paul Wild Observatory 899:coronal mass ejection 798:Qitai Radio Telescope 326:Meerkat National Park 302:Meerkat National Park 283:Meerkat National Park 240:Meerkat National Park 220:Meerkat National Park 151:Meerkat National Park 68: 56: 7567:Solar radio emission 7356:Jocelyn Bell Burnell 7214:Haystack Observatory 6748:Green Bank Telescope 6732:Effelsberg Telescope 6480:on 29 September 2015 6156:. September 18, 2017 5650:Parkes.atnf.csiro.au 5566:. 13 September 2023. 5552:. 13 September 2023. 4762:Green Bank Telescope 4494:Chinese Earth-Moon L 4440:Earth orbit with an 4395:Dunedin, New Zealand 4109:Cassegrain telescope 4002:La Silla Observatory 3463:Pie Town, New Mexico 3455:Brewster, Washington 3440:(operations center) 3013:Haystack Observatory 2938:Green Bank Telescope 2185:Bordeaux Observatory 2041:20 m telescope 2026:20 m telescope 2002:22 m telescope 1975:25 m telescope 1960:25 m telescope 1933:RT3 (15 m) antenna. 1918:Toruń RT3 15 m 1766:. Also includes the 1713:32 m VLBI dish 1688:32 m VLBI dish 1615:Toruń RT4 32 m 1149:University of Sydney 934:, Republic of Korea 917:327 MHz and 654 MHz 621:Ooty Radio Telescope 390:South Pole Telescope 35:adding missing items 7691:Lists of telescopes 7540:Pulsar timing array 7346:Edward George Bowen 7336:Elizabeth Alexander 7198:Arecibo Observatory 7102:Submillimeter Array 7004:Low-Frequency Array 6974:Korean VLBI Network 6840:Southern Hemisphere 6751:(West Virginia, US) 6531:on 24 December 2013 6403:2005ASPC..344..242K 6154:"CHIME First Light" 5115:on 10 December 2010 4926:Lists of telescopes 4641:Proposed telescopes 4404:University of Otago 4314:Submillimeter Array 4124:Studies of aurorae 4092:Greenland Telescope 3934:45 and 90 GHz 3874:NANTEN2 Observatory 3475:North Liberty, Iowa 3340:Stanford University 3065:Steward Observatory 2673:Steward Observatory 1057:array, operated by 660:, Karnataka, India 307:0.58–14.5 GHz 288:1200–1950 MHz 7520:Aperture synthesis 7489:Infrared astronomy 7426:Joseph Lade Pawsey 7396:Kenneth Kellermann 7366:Nan Dieter-Conklin 7074:One-Mile Telescope 6853:Parkes Observatory 6500:"TART Source Code" 5723:Iopscience.iop.org 5243:"Introducing GMRT" 5109:Astro.uchicago.edu 4703:Below 30 MHz 4107:12 metre diameter 4039:S/X/Ka, Delta Dor 3821:Lurigancho-Chosica 3799:Atibaia, São Paulo 3746:Cachoeira Paulista 3459:Kitt Peak, Arizona 2928:, and now kept by 2858:parabolic antennas 2853:408–1420 MHz 2620:0.5–11.5 GHz 2494:. 64 m dish. 2006:Simeiz Observatory 1981:Dwingeloo (CAMRAS) 1907:University of Bonn 1244:Parkes Observatory 1144:600–1200 MHz 1055:aperture synthesis 1015:700–1800 MHz 949:Republic of Korea 874:) operated by the 611:. Operated by the 198:2.3–8.65 GHz 75: 63: 33:; you can help by 7603: 7602: 7545:Radio propagation 7494:Optical astronomy 7391:Karl Guthe Jansky 7201:(Puerto Rico, US) 7176: 7175: 6968:West Virginia, US 6717:(Puerto Rico, US) 6714:Arecibo Telescope 5628:"Mopra telescope" 5421:www.miz.nao.ac.jp 5355:"FAST - Homepage" 5139:Pole.uchicago.edu 4976:Astro.caltech.edu 4810:parabolic antenna 4728: 4727: 4721:0.05–30 GHz 4638: 4637: 4613:0.3–117 GHz 4534: 4533: 4410: 4409: 4325:180–420 GHz 4245: 4244: 4208: 4207: 4184:Arecibo Telescope 4128: 4127: 4067: 4066: 3758:1.2–6.0 GHz 3652:159–738 GHz 3556:127–163 GHz 3513: 3512: 3471:Fort Davis, Texas 3447:Mauna Kea, Hawaii 3412:Array of 8 small 3329:, California, US 3323:Antenna Facility 3321:SRI International 3292:100–200 MHz 3080:100–200 MHz 2834:100–300 MHz 2763:since the 1970s. 2721:400–800 MHz 2697:4.5–5.5 GHz 2629:SRI International 2553: 2552: 2517:1.5–300 GHz 2451:ERAC Phased Array 2429:ERAC Phased Array 2412:(ERAC Telescope) 2316:150–450 MHz 2247:Plateau de Bure, 2228:Plateau de Bure, 2196:1.4–1.7 GHz 2187:radio telescope) 2178:12.8 m dish 1632:parabolic antenna 1573:radio telescope) 1426:0.61–30 GHz 1266: 1265: 1228:Western Australia 1176:0.3–100 GHz 1164:Mopra Observatory 1050:0.3–110 GHz 1011:Western Australia 975: 974: 789:70–3000 MHz 677:Nagano Prefecture 645:parabolic antenna 604:50–1420 MHz 415: 414: 342: 341: 331:100–200 MHz 245:400–800 MHz 177:1.66–23 GHz 156:4.5–5.5 GHz 51: 50: 7698: 7686:Radio telescopes 7668: 7667: 7666: 7656: 7655: 7654: 7644: 7643: 7642: 7632: 7631: 7620: 7619: 7618: 7611: 7593: 7592: 7583: 7582: 7560:HD 164595 signal 7535:Odd radio circle 7513:Related articles 7431:Ruby Payne-Scott 7361:Arthur Covington 7351:Ronald Bracewell 7321: 7313: 7305: 7286: 7277: 7267: 7258: 7250: 7242: 7234: 7226: 7218: 7210: 7202: 7194: 7168: 7158: 7137: 7127: 7117: 7112:Very Large Array 7107: 7097: 7087: 7078: 7069: 7059: 7049: 7039: 7029: 7019: 7009: 6999: 6989: 6988:Argentina/Brazil 6979: 6969: 6959: 6944: 6935: 6925: 6915: 6905: 6895: 6885: 6865: 6857: 6849: 6841: 6834: 6830:Yevpatoria RT-70 6826: 6818: 6810: 6802: 6793: 6784: 6776: 6768: 6764:Lovell Telescope 6760: 6752: 6744: 6736: 6727: 6718: 6709: 6692: 6681:Radio telescopes 6613: 6606: 6599: 6590: 6561: 6557: 6551: 6547: 6541: 6540: 6538: 6536: 6521: 6515: 6514: 6512: 6510: 6496: 6490: 6489: 6487: 6485: 6476:. Archived from 6466: 6457: 6456: 6454: 6453: 6438: 6432: 6431: 6429: 6428: 6419:. Archived from 6413: 6407: 6406: 6390: 6384: 6383: 6381: 6380: 6369: 6363: 6362: 6358: 6352: 6351: 6349: 6348: 6343:on July 23, 2010 6339:. Archived from 6333: 6327: 6326: 6324: 6323: 6309: 6303: 6302: 6284: 6274: 6250: 6244: 6243: 6241: 6240: 6226: 6220: 6219: 6217: 6216: 6205: 6199: 6198: 6191: 6185: 6184: 6182: 6181: 6171: 6165: 6164: 6162: 6161: 6150: 6144: 6143: 6141: 6139: 6125: 6119: 6118: 6096: 6090: 6089: 6087: 6085: 6071: 6065: 6064: 6062: 6060: 6046: 6040: 6039: 6037: 6035: 6021: 6015: 6014: 6012: 6011: 6002:. Archived from 5996: 5990: 5989: 5987: 5985: 5971: 5965: 5964: 5962: 5960: 5946: 5940: 5939: 5937: 5935: 5921: 5915: 5914: 5912: 5910: 5896: 5887: 5886: 5884: 5882: 5868: 5857: 5856: 5854: 5852: 5838: 5829: 5828: 5826: 5824: 5810: 5804: 5803: 5801: 5799: 5785: 5779: 5778: 5772: 5764: 5762: 5761: 5755: 5749:. Archived from 5748: 5740: 5734: 5733: 5731: 5729: 5720: 5712: 5703: 5702: 5696: 5688: 5686: 5685: 5676:. Archived from 5670: 5661: 5660: 5658: 5656: 5642: 5636: 5635: 5624: 5618: 5617: 5606: 5600: 5599: 5588: 5582: 5581: 5574: 5568: 5567: 5560: 5554: 5553: 5546: 5540: 5539: 5532: 5526: 5525: 5523: 5521: 5506: 5500: 5499: 5463: 5457: 5456: 5454: 5452: 5437: 5431: 5430: 5428: 5427: 5417:"Toppage - VERA" 5413: 5407: 5406: 5404: 5403: 5394:. Archived from 5388: 5382: 5377: 5371: 5370: 5368: 5366: 5361:on 16 March 2017 5351: 5345: 5344: 5338: 5330: 5328: 5327: 5321: 5315:. Archived from 5314: 5306: 5300: 5299: 5297: 5295: 5281: 5275: 5274: 5263: 5257: 5256: 5254: 5253: 5239: 5233: 5232: 5230: 5228: 5209: 5203: 5202: 5200: 5198: 5189: 5181: 5175: 5174: 5172: 5170: 5156: 5150: 5149: 5147: 5145: 5131: 5125: 5124: 5122: 5120: 5111:. Archived from 5101: 5095: 5094: 5087: 5081: 5080: 5078: 5077: 5068:. Archived from 5062: 5056: 5055: 5053: 5051: 5042:. Archived from 5032: 5026: 5025: 5023: 5021: 5010: 5004: 5003: 5001: 5000: 4986: 4980: 4979: 4968: 4959: 4958: 4947: 4897: 4881: 4861: 4846:Yevpatoria RT-70 4841: 4825: 4805: 4789: 4773: 4757: 4741: 4654:Frequency Range 4645: 4610:Xinjiang, China 4596:45–900 GHz 4550:Frequency Range 4541: 4426:Frequency Range 4417: 4367:Warkworth 2 dish 4355:1.2–21 GHz 4261:Frequency Range 4252: 4224:Frequency Range 4215: 4153:Very Small Array 4144:Frequency Range 4135: 4083:Frequency Range 4074: 4048:Malargüe Station 4034:Neuquén Province 4030: 3861:30–240 GHz 3529:Frequency Range 3520: 3392:. Part of NRAO. 3371:Very Large Array 2788:75–345 GHz 2625:gregorian offset 2569:Frequency Range 2560: 2379:0.4–22 GHz 2355:10–240 MHz 2320:NRH website (fr) 2298:DAM website (fr) 2294:10–100 MHz 2276:NRT website (fr) 2191:Floirac, Gironde 2047:Pluton (complex) 1828: 1726:0.3–86 GHz 1705:1.4–43 GHz 1561:1.4–22 GHz 1545:1.4–22 GHz 1367:Lovell Telescope 1282:Frequency Range 1273: 1232:70–300 MHz 1206:1.2–23 GHz 1113:1.2–23 GHz 991:Frequency Range 982: 937:86–115 GHz 894:150 MHz–450 MHz 889:Sichuan province 718:1.4–22 GHz 682:17–115 GHz 663:40–150 MHz 577:Shanghai, China 523:0.4–15 GHz 509:50–200 MHz 506:Xinjiang, China 488:1.4–18 GHz 471:Shanghai, China 454:85–115 GHz 431:Frequency Range 422: 400:95–350 GHz 358:Frequency Range 349: 225:50–200 MHz 180:26 m dish. 113:Frequency Range 104: 46: 43: 25: 24: 18: 7706: 7705: 7701: 7700: 7699: 7697: 7696: 7695: 7676: 7675: 7674: 7664: 7662: 7652: 7650: 7640: 7638: 7626: 7616: 7614: 7606: 7604: 7599: 7571: 7508: 7476: 7470: 7456:Gart Westerhout 7324: 7319: 7311: 7303: 7289: 7284: 7275: 7265: 7264:(PRAO ASC LPI, 7256: 7248: 7240: 7232: 7224: 7216: 7208: 7200: 7192: 7172: 7166: 7156: 7141: 7135: 7125: 7115: 7105: 7095: 7085: 7076: 7067: 7057: 7047: 7037: 7027: 7017: 7007: 6997: 6987: 6977: 6967: 6957: 6942: 6933: 6923: 6913: 6903: 6893: 6883: 6873:Interferometers 6868: 6863: 6855: 6847: 6839: 6832: 6824: 6816: 6814:Usuda Telescope 6808: 6800: 6791: 6782: 6774: 6766: 6758: 6750: 6742: 6734: 6725: 6716: 6707: 6696: 6683: 6675: 6645:Radio telescope 6622: 6620:Radio astronomy 6617: 6570: 6565: 6564: 6558: 6554: 6548: 6544: 6534: 6532: 6523: 6522: 6518: 6508: 6506: 6498: 6497: 6493: 6483: 6481: 6474:Irasr.aut.ac.nz 6468: 6467: 6460: 6451: 6449: 6440: 6439: 6435: 6426: 6424: 6415: 6414: 6410: 6392: 6391: 6387: 6378: 6376: 6371: 6370: 6366: 6360: 6359: 6355: 6346: 6344: 6335: 6334: 6330: 6321: 6319: 6311: 6310: 6306: 6252: 6251: 6247: 6238: 6236: 6228: 6227: 6223: 6214: 6212: 6207: 6206: 6202: 6193: 6192: 6188: 6179: 6177: 6173: 6172: 6168: 6159: 6157: 6152: 6151: 6147: 6137: 6135: 6127: 6126: 6122: 6107: 6104:Wayback Machine 6097: 6093: 6083: 6081: 6073: 6072: 6068: 6058: 6056: 6048: 6047: 6043: 6033: 6031: 6023: 6022: 6018: 6009: 6007: 6000:"Wurzburg v2.0" 5998: 5997: 5993: 5983: 5981: 5973: 5972: 5968: 5958: 5956: 5948: 5947: 5943: 5933: 5931: 5929:Nrw-stiftung.de 5923: 5922: 5918: 5908: 5906: 5898: 5897: 5890: 5880: 5878: 5870: 5869: 5860: 5850: 5848: 5840: 5839: 5832: 5822: 5820: 5812: 5811: 5807: 5797: 5795: 5787: 5786: 5782: 5765: 5759: 5757: 5753: 5746: 5744:"Archived copy" 5742: 5741: 5737: 5727: 5725: 5718: 5714: 5713: 5706: 5689: 5683: 5681: 5674:"Archived copy" 5672: 5671: 5664: 5654: 5652: 5644: 5643: 5639: 5634:. 6 April 2021. 5626: 5625: 5621: 5608: 5607: 5603: 5590: 5589: 5585: 5576: 5575: 5571: 5562: 5561: 5557: 5548: 5547: 5543: 5534: 5533: 5529: 5519: 5517: 5508: 5507: 5503: 5465: 5464: 5460: 5450: 5448: 5439: 5438: 5434: 5425: 5423: 5415: 5414: 5410: 5401: 5399: 5390: 5389: 5385: 5378: 5374: 5364: 5362: 5353: 5352: 5348: 5331: 5325: 5323: 5319: 5312: 5310:"Archived copy" 5308: 5307: 5303: 5293: 5291: 5283: 5282: 5278: 5265: 5264: 5260: 5251: 5249: 5241: 5240: 5236: 5226: 5224: 5211: 5210: 5206: 5196: 5194: 5187: 5183: 5182: 5178: 5168: 5166: 5158: 5157: 5153: 5143: 5141: 5133: 5132: 5128: 5118: 5116: 5103: 5102: 5098: 5089: 5088: 5084: 5075: 5073: 5066:"About the KAT" 5064: 5063: 5059: 5049: 5047: 5046:on 5 March 2012 5034: 5033: 5029: 5019: 5017: 5012: 5011: 5007: 4998: 4996: 4988: 4987: 4983: 4970: 4969: 4962: 4949: 4948: 4944: 4939: 4931:Radio telescope 4912: 4905: 4898: 4889: 4882: 4873: 4862: 4853: 4842: 4833: 4826: 4817: 4806: 4797: 4790: 4781: 4774: 4765: 4758: 4749: 4742: 4733: 4681:10–80 MHz 4678:Nançay, France 4643: 4539: 4497: 4476:or RadioAstron 4415: 4399:1.575 GHz 4250: 4213: 4133: 4072: 4024: 3734:emission line. 3724:crossed-dragone 3688:silicon nitride 3518: 3439: 3336:U.S. Government 3151:10–88 MHz 2761:carbon monoxide 2558: 2485:Sardinia, Italy 2128:2–150 GHz 1886:25 m dish 1857:superheterodyne 1822: 1740:United Kingdom 1404:5–300 GHz 1384:76 m dish 1271: 1248:New South Wales 1172:New South Wales 1109:South Australia 1073: 1046:New South Wales 1033: 1002: 980: 872:Ishigaki island 766:5–300 GHz 741:5–300 GHz 641:radio telescope 636:326.5 MHz 569:Built in 2006. 563:Kunming, China 555:Built in 2005. 440:Delingha 13.7 m 420: 377:26–36 GHz 347: 328:, South Africa 304:, South Africa 285:, South Africa 242:, South Africa 222:, South Africa 195:, South Africa 174:, South Africa 153:, South Africa 102: 91:interferometric 83:radio astronomy 47: 41: 38: 22: 12: 11: 5: 7704: 7702: 7694: 7693: 7688: 7678: 7677: 7673: 7672: 7660: 7648: 7636: 7624: 7601: 7600: 7598: 7597: 7587: 7576: 7573: 7572: 7570: 7569: 7564: 7563: 7562: 7557: 7547: 7542: 7537: 7532: 7530:Interferometry 7527: 7522: 7516: 7514: 7510: 7509: 7507: 7506: 7501: 7496: 7491: 7486: 7480: 7478: 7472: 7471: 7469: 7468: 7463: 7458: 7453: 7448: 7443: 7438: 7433: 7428: 7423: 7418: 7413: 7411:Bernard Lovell 7408: 7403: 7398: 7393: 7388: 7383: 7378: 7373: 7368: 7363: 7358: 7353: 7348: 7343: 7341:John G. Bolton 7338: 7332: 7330: 7326: 7325: 7323: 7322: 7314: 7309:ESA New Norcia 7306: 7297: 7295: 7291: 7290: 7288: 7287: 7279: 7269: 7259: 7251: 7243: 7235: 7227: 7219: 7211: 7203: 7195: 7186: 7184: 7178: 7177: 7174: 7173: 7171: 7170: 7160: 7149: 7147: 7143: 7142: 7140: 7139: 7129: 7119: 7116:New Mexico, US 7109: 7099: 7089: 7079: 7071: 7061: 7051: 7041: 7031: 7021: 7011: 7001: 6998:New Mexico, US 6991: 6981: 6971: 6961: 6951: 6945: 6937: 6934:California, US 6927: 6917: 6907: 6897: 6887: 6884:California, US 6876: 6874: 6870: 6869: 6867: 6866: 6858: 6850: 6848:(South Africa) 6842: 6836: 6835: 6827: 6819: 6811: 6803: 6795: 6785: 6777: 6772:Ooty Telescope 6769: 6761: 6753: 6745: 6737: 6729: 6719: 6711: 6700: 6698: 6689: 6677: 6676: 6674: 6673: 6668: 6662: 6652: 6642: 6630: 6628: 6624: 6623: 6618: 6616: 6615: 6608: 6601: 6593: 6587: 6586: 6581: 6576: 6569: 6568:External links 6566: 6563: 6562: 6552: 6542: 6516: 6491: 6458: 6433: 6408: 6385: 6364: 6353: 6328: 6304: 6245: 6234:www.lmtgtm.org 6221: 6200: 6186: 6166: 6145: 6120: 6091: 6066: 6041: 6016: 5991: 5966: 5954:Astropeiler.de 5941: 5916: 5888: 5858: 5842:"Meteoriti.LV" 5830: 5805: 5780: 5735: 5704: 5662: 5637: 5619: 5614:Cdscc.nasa.gov 5601: 5583: 5569: 5555: 5541: 5527: 5516:. 29 June 2022 5501: 5458: 5432: 5408: 5383: 5372: 5346: 5301: 5276: 5258: 5234: 5223:on 4 June 2015 5204: 5176: 5164:Eurekalert.org 5151: 5126: 5096: 5082: 5057: 5027: 5005: 4981: 4960: 4941: 4940: 4938: 4935: 4934: 4933: 4928: 4923: 4918: 4911: 4908: 4907: 4906: 4899: 4892: 4890: 4883: 4876: 4874: 4863: 4856: 4854: 4843: 4836: 4834: 4827: 4820: 4818: 4807: 4800: 4798: 4791: 4784: 4782: 4776:The 100 meter 4775: 4768: 4766: 4760:The 100 meter 4759: 4752: 4750: 4744:The 500 meter 4743: 4736: 4732: 4729: 4726: 4725: 4722: 4719: 4716: 4709: 4708: 4704: 4701: 4698: 4691: 4690: 4682: 4679: 4676: 4672: 4671: 4668: 4666: 4663: 4659: 4658: 4655: 4652: 4649: 4642: 4639: 4636: 4635: 4632: 4629: 4626: 4619: 4618: 4614: 4611: 4608: 4601: 4600: 4597: 4594: 4581: 4574: 4573: 4570: 4569:0–11 GHz 4567: 4564:Cambridgeshire 4561: 4555: 4554: 4551: 4548: 4545: 4538: 4535: 4532: 4531: 4529: 4527: 4524: 4518: 4517: 4515: 4513: 4510: 4504: 4503: 4501: 4499: 4495: 4492: 4486: 4485: 4482: 4480: 4477: 4470: 4469: 4466: 4464: 4461: 4455: 4454: 4451: 4449: 4438: 4431: 4430: 4427: 4424: 4421: 4414: 4411: 4408: 4407: 4400: 4397: 4391: 4385: 4384: 4381: 4380:6–21 GHz 4378: 4369: 4363: 4362: 4356: 4353: 4344: 4338: 4337: 4326: 4323: 4317: 4310: 4309: 4303: 4300: 4290: 4284: 4283: 4280: 4278: 4272: 4266: 4265: 4262: 4259: 4256: 4249: 4246: 4243: 4242: 4240: 4235: 4229: 4228: 4225: 4222: 4219: 4212: 4209: 4206: 4205: 4202:radiotelescope 4198: 4195: 4186: 4180: 4179: 4168: 4166: 4163:Canary Islands 4156: 4149: 4148: 4145: 4142: 4139: 4132: 4131:Atlantic Ocean 4129: 4126: 4125: 4122: 4120: 4117: 4113: 4112: 4105: 4103: 4097:Thule Air Base 4094: 4088: 4087: 4084: 4081: 4078: 4071: 4068: 4065: 4064: 4058: 4056: 4050: 4044: 4043: 4040: 4037: 4031: 4018: 4017: 4014: 4012: 4006:Atacama Desert 3999: 3992: 3991: 3984: 3981: 3972: 3965: 3964: 3961: 3959: 3953:Atacama Desert 3946: 3939: 3938: 3935: 3932: 3923: 3917: 3916: 3913: 3911: 3902: 3896: 3895: 3892: 3890: 3884:Atacama Desert 3877: 3870: 3869: 3862: 3859: 3853:Atacama Desert 3846: 3839: 3838: 3834: 3831: 3818: 3811: 3810: 3807: 3805: 3796: 3790: 3789: 3786: 3784: 3778:Atacama Desert 3771: 3764: 3763: 3759: 3756: 3743: 3736: 3735: 3720: 3717: 3703: 3696: 3695: 3680: 3677: 3671:Atacama Desert 3664: 3657: 3656: 3653: 3650: 3644:Atacama Desert 3637: 3630: 3629: 3614: 3611: 3605:Atacama Desert 3598: 3591: 3590: 3587: 3585: 3579:Atacama Desert 3572: 3565: 3564: 3557: 3554: 3548:Atacama Desert 3541: 3534: 3533: 3530: 3527: 3524: 3517: 3514: 3511: 3510: 3507: 3504: 3501:North Carolina 3494: 3487: 3486: 3443: 3441: 3429: 3422: 3421: 3410: 3408: 3398: 3394: 3393: 3386: 3384: 3374: 3367: 3366: 3363: 3361: 3351: 3349:interferometer 3344: 3343: 3332: 3330: 3324: 3317: 3316: 3313: 3311: 3301: 3297: 3296: 3293: 3290: 3280: 3273: 3272: 3265: 3263: 3253: 3247: 3246: 3235: 3232: 3218: 3212: 3211: 3208: 3206: 3203: 3199: 3198: 3195: 3193: 3190: 3186: 3185: 3182: 3180: 3170: 3164: 3163: 3152: 3149: 3139: 3133: 3132: 3126: 3124: 3114: 3108: 3107: 3104: 3102: 3092: 3085: 3084: 3081: 3078: 3075: 3069: 3068: 3054: 3052: 3042: 3035: 3034: 3027: 3025: 3015: 3009: 3008: 2998: 2996: 2986: 2982: 2981: 2978: 2975: 2965: 2958: 2957: 2954: 2951: 2941: 2934: 2933: 2922: 2920: 2910: 2903: 2902: 2899: 2897: 2894: 2888: 2887: 2881: 2879: 2869: 2862: 2861: 2854: 2851: 2845: 2839: 2838: 2835: 2832: 2826: 2820: 2819: 2793:interferometer 2791:Heterogeneous 2789: 2786: 2772: 2765: 2764: 2757: 2754: 2744: 2738: 2737: 2722: 2719: 2709: 2702: 2701: 2698: 2695: 2681: 2677: 2676: 2658: 2656: 2642: 2636: 2635: 2633:SETI Institute 2621: 2618: 2604: 2598: 2597: 2594: 2592: 2585:Algonquin Park 2578: 2574: 2573: 2570: 2567: 2564: 2557: 2554: 2551: 2550: 2544: 2541: 2532: 2526: 2525: 2518: 2515: 2502: 2496: 2495: 2489: 2487: 2478: 2472: 2471: 2468: 2466: 2453: 2447: 2446: 2443: 2441: 2431: 2425: 2424: 2421: 2419: 2413: 2406: 2405: 2402: 2400: 2390: 2384: 2383: 2380: 2377: 2371: 2364: 2363: 2356: 2353: 2350: 2343: 2342: 2335: 2333: 2330: 2323: 2322: 2317: 2314: 2308: 2301: 2300: 2295: 2292: 2286: 2279: 2278: 2273: 2271: 2265: 2258: 2257: 2254: 2252: 2245: 2239: 2238: 2235: 2233: 2226: 2220: 2219: 2213: 2211: 2208: 2201: 2200: 2197: 2194: 2188: 2180: 2179: 2176: 2174: 2165: 2159: 2158: 2151: 2149: 2139: 2137:Ryle Telescope 2133: 2132: 2129: 2126: 2116: 2110: 2109: 2106: 2104: 2094: 2088: 2087: 2084: 2082: 2069: 2065: 2064: 2061: 2059: 2049: 2043: 2042: 2039: 2037: 2027: 2023: 2022: 2018: 2016: 2003: 1999: 1998: 1991: 1989: 1988:, Netherlands 1983: 1977: 1976: 1973: 1971: 1961: 1957: 1956: 1950: 1948: 1947:, Netherlands 1942: 1935: 1934: 1931: 1929: 1919: 1915: 1914: 1903: 1901: 1894: 1888: 1887: 1884: 1883:0–24 GHz 1881: 1871: 1865: 1864: 1849: 1847: 1837: 1831: 1830: 1817: 1815: 1805: 1799: 1798: 1795: 1794:0–11 GHz 1792: 1789:Cambridgeshire 1786: 1780: 1779: 1774:telescopes at 1744: 1741: 1738: 1731: 1730: 1727: 1724: 1714: 1710: 1709: 1706: 1703: 1689: 1685: 1684: 1681: 1678: 1664: 1658: 1657: 1654: 1652: 1639: 1635: 1634: 1628: 1626: 1616: 1612: 1611: 1608: 1606: 1592: 1586: 1585: 1582: 1580: 1574: 1566: 1565: 1562: 1559: 1556: 1552: 1551: 1546: 1543: 1540: 1538:Zelenchukskaya 1533: 1532: 1525: 1523: 1517: 1513: 1512: 1504: 1502: 1496: 1492: 1491: 1483: 1481: 1475: 1471: 1470: 1467: 1466:5.86 GHz 1464: 1458: 1451: 1450: 1447: 1446:5.86 GHz 1444: 1438: 1431: 1430: 1427: 1424: 1421:Zelenchukskaya 1418: 1412: 1411: 1405: 1402: 1392: 1386: 1385: 1382: 1379: 1369: 1363: 1362: 1359: 1358:8–80 MHz 1356: 1348:Volokhiv Yar, 1346: 1339: 1338: 1331: 1330:8–33 MHz 1328: 1320:Volokhiv Yar, 1318: 1311: 1310: 1303: 1300: 1293: 1287: 1286: 1283: 1280: 1277: 1270: 1267: 1264: 1263: 1252: 1250: 1241: 1237: 1236: 1233: 1230: 1221: 1214: 1213: 1207: 1204: 1195: 1189: 1188: 1177: 1174: 1161: 1157: 1156: 1145: 1142: 1128: 1121: 1120: 1114: 1111: 1102: 1098: 1097: 1086: 1084: 1075: 1067: 1066: 1051: 1048: 1035: 1027: 1026: 1016: 1013: 1004: 996: 995: 992: 989: 986: 979: 976: 973: 972: 953: 950: 947: 943: 942: 938: 935: 929: 925: 924: 918: 915: 912:Inner Mongolia 909: 903: 902: 895: 892: 886: 880: 879: 856: 853: 850: 844: 843: 836: 833: 827: 821: 820: 813: 810: 800: 794: 793: 790: 787: 781: 774: 773: 767: 764: 755: 749: 748: 742: 739: 729: 723: 722: 719: 716: 713: 709: 708: 704: 701: 698: 691: 690: 683: 680: 674: 668: 667: 664: 661: 655: 649: 648: 637: 634: 624: 617: 616: 605: 602: 592: 585: 584: 581: 580:1–50 GHz 578: 575: 571: 570: 567: 566:2–12 GHz 564: 561: 557: 556: 553: 552:2–12 GHz 550: 547: 543: 542: 539: 536: 533: 529: 528: 524: 521: 518: 514: 513: 510: 507: 504: 497: 496: 489: 486: 485:Ürümqi, China 483: 479: 478: 475: 474:1660 MHz 472: 469: 463: 462: 455: 452: 442: 436: 435: 432: 429: 426: 419: 416: 413: 412: 411:observations. 401: 398: 393: 386: 385: 378: 375: 370: 363: 362: 359: 356: 353: 346: 343: 340: 339: 336:interferometer 332: 329: 323: 316: 315: 308: 305: 299: 293: 292: 289: 286: 280: 274: 273: 270: 269:1420 MHz 267: 254: 250: 249: 246: 243: 237: 230: 229: 226: 223: 217: 210: 209: 199: 196: 186: 182: 181: 178: 175: 165: 161: 160: 157: 154: 148: 141: 140: 133: 130: 124: 118: 117: 114: 111: 108: 101: 98: 49: 48: 28: 26: 13: 10: 9: 6: 4: 3: 2: 7703: 7692: 7689: 7687: 7684: 7683: 7681: 7671: 7661: 7659: 7649: 7647: 7637: 7635: 7630: 7625: 7623: 7613: 7609: 7596: 7588: 7586: 7578: 7577: 7574: 7568: 7565: 7561: 7558: 7556: 7553: 7552: 7551: 7548: 7546: 7543: 7541: 7538: 7536: 7533: 7531: 7528: 7526: 7523: 7521: 7518: 7517: 7515: 7511: 7505: 7502: 7500: 7497: 7495: 7492: 7490: 7487: 7485: 7482: 7481: 7479: 7473: 7467: 7466:Robert Wilson 7464: 7462: 7459: 7457: 7454: 7452: 7451:Govind Swarup 7449: 7447: 7444: 7442: 7439: 7437: 7434: 7432: 7429: 7427: 7424: 7422: 7419: 7417: 7414: 7412: 7409: 7407: 7406:John D. Kraus 7404: 7402: 7401:Frank J. Kerr 7399: 7397: 7394: 7392: 7389: 7387: 7384: 7382: 7381:Antony Hewish 7379: 7377: 7374: 7372: 7369: 7367: 7364: 7362: 7359: 7357: 7354: 7352: 7349: 7347: 7344: 7342: 7339: 7337: 7334: 7333: 7331: 7327: 7318: 7315: 7310: 7307: 7302: 7299: 7298: 7296: 7292: 7283: 7280: 7273: 7270: 7263: 7260: 7255: 7252: 7247: 7244: 7239: 7236: 7231: 7228: 7223: 7220: 7215: 7212: 7207: 7204: 7199: 7196: 7191: 7188: 7187: 7185: 7183: 7182:Observatories 7179: 7164: 7161: 7154: 7151: 7150: 7148: 7144: 7133: 7130: 7123: 7120: 7113: 7110: 7103: 7100: 7093: 7090: 7083: 7080: 7075: 7072: 7065: 7062: 7055: 7052: 7045: 7042: 7035: 7032: 7025: 7022: 7015: 7012: 7005: 7002: 6995: 6992: 6985: 6982: 6975: 6972: 6965: 6962: 6955: 6952: 6949: 6946: 6941: 6938: 6931: 6928: 6921: 6918: 6911: 6908: 6901: 6898: 6891: 6888: 6881: 6878: 6877: 6875: 6871: 6862: 6859: 6854: 6851: 6846: 6843: 6838: 6837: 6831: 6828: 6823: 6820: 6815: 6812: 6807: 6804: 6799: 6796: 6789: 6786: 6781: 6778: 6773: 6770: 6765: 6762: 6757: 6754: 6749: 6746: 6741: 6740:Galenki RT-70 6738: 6733: 6730: 6723: 6720: 6715: 6712: 6705: 6702: 6701: 6699: 6693: 6690: 6687: 6682: 6678: 6672: 6669: 6666: 6663: 6660: 6656: 6653: 6650: 6646: 6643: 6640: 6636: 6632: 6631: 6629: 6625: 6621: 6614: 6609: 6607: 6602: 6600: 6595: 6594: 6591: 6585: 6582: 6580: 6577: 6575: 6572: 6571: 6567: 6560: 6556: 6553: 6550: 6546: 6543: 6530: 6526: 6520: 6517: 6505: 6501: 6495: 6492: 6479: 6475: 6471: 6465: 6463: 6459: 6447: 6443: 6437: 6434: 6423:on 2012-07-30 6422: 6418: 6412: 6409: 6404: 6400: 6396: 6389: 6386: 6374: 6368: 6365: 6357: 6354: 6342: 6338: 6332: 6329: 6318: 6314: 6308: 6305: 6300: 6296: 6292: 6288: 6283: 6278: 6273: 6268: 6264: 6260: 6256: 6249: 6246: 6235: 6231: 6225: 6222: 6210: 6204: 6201: 6196: 6195:"ALMA Basics" 6190: 6187: 6176: 6170: 6167: 6155: 6149: 6146: 6134: 6133:169.48.13.120 6130: 6124: 6121: 6116: 6115: 6110: 6105: 6101: 6095: 6092: 6080: 6076: 6070: 6067: 6055: 6051: 6045: 6042: 6030: 6026: 6020: 6017: 6006:on 2013-05-10 6005: 6001: 5995: 5992: 5980: 5976: 5970: 5967: 5955: 5951: 5945: 5942: 5930: 5926: 5920: 5917: 5905: 5901: 5895: 5893: 5889: 5877: 5873: 5867: 5865: 5863: 5859: 5847: 5843: 5837: 5835: 5831: 5819: 5815: 5809: 5806: 5794: 5790: 5784: 5781: 5776: 5770: 5756:on 2010-05-13 5752: 5745: 5739: 5736: 5724: 5717: 5711: 5709: 5705: 5700: 5694: 5680:on 2008-12-26 5679: 5675: 5669: 5667: 5663: 5651: 5647: 5641: 5638: 5633: 5629: 5623: 5620: 5615: 5611: 5605: 5602: 5597: 5593: 5587: 5584: 5579: 5573: 5570: 5565: 5559: 5556: 5551: 5545: 5542: 5537: 5531: 5528: 5515: 5511: 5505: 5502: 5497: 5493: 5489: 5485: 5481: 5477: 5473: 5469: 5462: 5459: 5447:. 5 July 2022 5446: 5442: 5436: 5433: 5422: 5418: 5412: 5409: 5398:on 2019-06-23 5397: 5393: 5387: 5384: 5381: 5376: 5373: 5360: 5356: 5350: 5347: 5342: 5336: 5322:on 2010-02-14 5318: 5311: 5305: 5302: 5290: 5289:Wikimapia.org 5286: 5280: 5277: 5272: 5268: 5262: 5259: 5248: 5244: 5238: 5235: 5222: 5218: 5214: 5208: 5205: 5193: 5192:Atnf.csiro.au 5186: 5180: 5177: 5165: 5161: 5155: 5152: 5140: 5136: 5130: 5127: 5114: 5110: 5106: 5100: 5097: 5092: 5086: 5083: 5072:on 2007-02-08 5071: 5067: 5061: 5058: 5045: 5041: 5037: 5031: 5028: 5015: 5009: 5006: 4995: 4994:Hartrao.ac.za 4991: 4985: 4982: 4977: 4973: 4967: 4965: 4961: 4956: 4952: 4946: 4943: 4936: 4932: 4929: 4927: 4924: 4922: 4919: 4917: 4914: 4913: 4909: 4903: 4896: 4891: 4887: 4880: 4875: 4871: 4867: 4866:Galenki RT-70 4864:The 70 meter 4860: 4855: 4851: 4847: 4844:The 70 meter 4840: 4835: 4831: 4824: 4819: 4815: 4811: 4804: 4799: 4795: 4792:The 76 meter 4788: 4783: 4779: 4772: 4767: 4763: 4756: 4751: 4747: 4740: 4735: 4730: 4723: 4720: 4717: 4715:(SKA-Phase2) 4714: 4711: 4710: 4705: 4702: 4699: 4696: 4693: 4692: 4687: 4683: 4680: 4677: 4674: 4673: 4669: 4667: 4664: 4661: 4660: 4656: 4653: 4650: 4647: 4646: 4640: 4633: 4630: 4627: 4625:(SKA-Phase1) 4624: 4621: 4620: 4615: 4612: 4609: 4606: 4603: 4602: 4598: 4595: 4593: 4589: 4585: 4582: 4579: 4576: 4575: 4571: 4568: 4565: 4562: 4560: 4557: 4556: 4552: 4549: 4546: 4543: 4542: 4536: 4530: 4528: 4525: 4523: 4520: 4519: 4516: 4514: 4511: 4509: 4506: 4505: 4502: 4500: 4493: 4491: 4488: 4487: 4483: 4481: 4478: 4475: 4472: 4471: 4467: 4465: 4462: 4460: 4457: 4456: 4452: 4450: 4447: 4443: 4439: 4436: 4433: 4432: 4428: 4425: 4422: 4419: 4418: 4412: 4405: 4401: 4398: 4396: 4393:Signal Hill, 4392: 4390: 4387: 4386: 4382: 4379: 4377: 4373: 4370: 4368: 4365: 4364: 4361: 4357: 4354: 4352: 4348: 4345: 4343: 4340: 4339: 4335: 4331: 4327: 4324: 4322:, Hawaii, US 4321: 4318: 4315: 4312: 4311: 4308: 4304: 4301: 4298: 4294: 4291: 4289: 4286: 4285: 4281: 4279: 4277:, Hawaii, US 4276: 4273: 4271: 4268: 4267: 4263: 4260: 4257: 4254: 4253: 4248:Pacific Ocean 4247: 4241: 4239: 4236: 4234: 4231: 4230: 4226: 4223: 4220: 4217: 4216: 4210: 4203: 4199: 4196: 4194: 4190: 4187: 4185: 4182: 4181: 4177: 4173: 4169: 4167: 4164: 4160: 4157: 4154: 4151: 4150: 4146: 4143: 4140: 4137: 4136: 4130: 4123: 4121: 4118: 4115: 4114: 4110: 4106: 4104: 4102: 4098: 4095: 4093: 4090: 4089: 4085: 4082: 4079: 4076: 4075: 4069: 4063: 4059: 4057: 4054: 4051: 4049: 4046: 4045: 4041: 4038: 4035: 4032: 4028: 4023: 4020: 4019: 4015: 4013: 4011: 4007: 4003: 4000: 3997: 3994: 3993: 3989: 3985: 3982: 3980: 3976: 3973: 3970: 3967: 3966: 3962: 3960: 3958: 3954: 3950: 3947: 3944: 3941: 3940: 3936: 3933: 3931: 3927: 3924: 3922: 3919: 3918: 3914: 3912: 3910: 3906: 3903: 3901: 3898: 3897: 3893: 3891: 3889: 3885: 3881: 3878: 3875: 3872: 3871: 3867: 3863: 3860: 3858: 3854: 3850: 3847: 3844: 3841: 3840: 3835: 3833:50 MHz 3832: 3830: 3826: 3825:Lima Province 3822: 3819: 3816: 3813: 3812: 3808: 3806: 3804: 3800: 3797: 3795: 3792: 3791: 3787: 3785: 3783: 3779: 3775: 3772: 3769: 3766: 3765: 3760: 3757: 3755: 3751: 3747: 3744: 3741: 3738: 3737: 3733: 3729: 3725: 3721: 3719:980-1260 MHz 3718: 3715: 3711: 3707: 3704: 3701: 3698: 3697: 3693: 3689: 3685: 3681: 3679:270 GHz 3678: 3676: 3672: 3668: 3665: 3662: 3659: 3658: 3654: 3651: 3649: 3645: 3641: 3638: 3635: 3632: 3631: 3627: 3623: 3619: 3615: 3612: 3610: 3606: 3602: 3599: 3596: 3593: 3592: 3588: 3586: 3584: 3580: 3576: 3573: 3570: 3567: 3566: 3562: 3558: 3555: 3553: 3549: 3545: 3542: 3539: 3536: 3535: 3531: 3528: 3525: 3522: 3521: 3516:South America 3515: 3508: 3505: 3502: 3498: 3495: 3492: 3489: 3488: 3484: 3480: 3476: 3472: 3468: 3464: 3460: 3456: 3452: 3448: 3444: 3442: 3437: 3433: 3430: 3427: 3424: 3423: 3419: 3415: 3411: 3409: 3406: 3402: 3401:Cogan Station 3399: 3396: 3395: 3391: 3387: 3385: 3382: 3378: 3375: 3372: 3369: 3368: 3364: 3362: 3359: 3355: 3352: 3350: 3346: 3345: 3341: 3337: 3333: 3331: 3328: 3325: 3322: 3319: 3318: 3314: 3312: 3309: 3305: 3302: 3299: 3298: 3294: 3291: 3288: 3287:West Virginia 3284: 3281: 3278: 3275: 3274: 3270: 3266: 3264: 3261: 3257: 3254: 3252: 3249: 3248: 3244: 3240: 3236: 3233: 3230: 3226: 3222: 3219: 3217: 3214: 3213: 3209: 3207: 3204: 3201: 3200: 3196: 3194: 3191: 3188: 3187: 3183: 3181: 3178: 3174: 3171: 3169: 3166: 3165: 3161: 3157: 3153: 3150: 3147: 3143: 3140: 3138: 3135: 3134: 3131: 3127: 3125: 3122: 3118: 3115: 3113: 3110: 3109: 3105: 3103: 3100: 3096: 3093: 3090: 3087: 3086: 3082: 3079: 3076: 3074: 3071: 3070: 3066: 3062: 3059: 3055: 3053: 3050: 3046: 3043: 3040: 3037: 3036: 3033: 3028: 3026: 3023: 3022:Massachusetts 3019: 3016: 3014: 3011: 3010: 3006: 3003: 2999: 2997: 2994: 2993:West Virginia 2990: 2987: 2984: 2983: 2979: 2976: 2973: 2972:West Virginia 2969: 2966: 2963: 2960: 2959: 2955: 2952: 2949: 2948:West Virginia 2945: 2942: 2939: 2936: 2935: 2931: 2927: 2923: 2921: 2918: 2917:West Virginia 2914: 2911: 2908: 2905: 2904: 2900: 2898: 2895: 2893: 2890: 2889: 2886: 2885:UMass Amherst 2882: 2880: 2877: 2876:Massachusetts 2873: 2870: 2867: 2864: 2863: 2859: 2855: 2852: 2849: 2846: 2844: 2841: 2840: 2836: 2833: 2830: 2827: 2825: 2822: 2821: 2817: 2813: 2809: 2805: 2801: 2798: 2794: 2790: 2787: 2784: 2780: 2776: 2773: 2770: 2767: 2766: 2762: 2758: 2756:115 GHz 2755: 2752: 2748: 2745: 2743: 2740: 2739: 2735: 2731: 2727: 2723: 2720: 2717: 2713: 2710: 2707: 2704: 2703: 2699: 2696: 2693: 2689: 2685: 2682: 2680:C-BASS North 2679: 2678: 2674: 2670: 2667: 2663: 2659: 2657: 2654: 2650: 2646: 2643: 2641: 2638: 2637: 2634: 2630: 2626: 2622: 2619: 2616: 2612: 2608: 2605: 2603: 2600: 2599: 2595: 2593: 2590: 2586: 2582: 2579: 2576: 2575: 2571: 2568: 2565: 2562: 2561: 2556:North America 2555: 2549: 2545: 2543:1.4 GHz 2542: 2540: 2536: 2535:Hertfordshire 2533: 2531: 2528: 2527: 2524: 2519: 2516: 2514: 2510: 2506: 2505:Mount Aragats 2503: 2501: 2498: 2497: 2493: 2490: 2488: 2486: 2482: 2479: 2477: 2474: 2473: 2469: 2467: 2465: 2461: 2457: 2454: 2452: 2449: 2448: 2444: 2442: 2439: 2435: 2432: 2430: 2427: 2426: 2422: 2420: 2417: 2414: 2411: 2408: 2407: 2403: 2401: 2398: 2394: 2391: 2389: 2386: 2385: 2381: 2378: 2375: 2372: 2369: 2366: 2365: 2362: 2357: 2354: 2351: 2348: 2345: 2344: 2340: 2336: 2334: 2331: 2328: 2325: 2324: 2321: 2318: 2315: 2312: 2309: 2306: 2303: 2302: 2299: 2296: 2293: 2290: 2287: 2284: 2281: 2280: 2277: 2274: 2272: 2269: 2266: 2263: 2260: 2259: 2255: 2253: 2250: 2246: 2244: 2241: 2240: 2236: 2234: 2231: 2227: 2225: 2222: 2221: 2218: 2214: 2212: 2209: 2206: 2203: 2202: 2198: 2195: 2192: 2189: 2186: 2182: 2181: 2177: 2175: 2173: 2169: 2166: 2164: 2161: 2160: 2156: 2152: 2150: 2147: 2143: 2140: 2138: 2135: 2134: 2130: 2127: 2124: 2120: 2117: 2115: 2112: 2111: 2107: 2105: 2102: 2098: 2095: 2093: 2090: 2089: 2085: 2083: 2081: 2077: 2073: 2070: 2067: 2066: 2062: 2060: 2058: 2054: 2050: 2048: 2045: 2044: 2040: 2038: 2035: 2031: 2028: 2025: 2024: 2019: 2017: 2015: 2011: 2007: 2004: 2001: 2000: 1996: 1992: 1990: 1987: 1984: 1982: 1979: 1978: 1974: 1972: 1969: 1965: 1962: 1959: 1958: 1955: 1951: 1949: 1946: 1943: 1940: 1937: 1936: 1932: 1930: 1927: 1923: 1920: 1917: 1916: 1912: 1908: 1904: 1902: 1899: 1895: 1893: 1890: 1889: 1885: 1882: 1879: 1875: 1872: 1870: 1867: 1866: 1862: 1858: 1854: 1850: 1848: 1845: 1841: 1838: 1836: 1833: 1832: 1826: 1821: 1818: 1816: 1814: 1810: 1806: 1804: 1801: 1800: 1796: 1793: 1790: 1787: 1785: 1782: 1781: 1777: 1773: 1769: 1765: 1761: 1757: 1753: 1749: 1745: 1742: 1739: 1736: 1733: 1732: 1728: 1725: 1722: 1718: 1715: 1712: 1711: 1707: 1704: 1701: 1697: 1693: 1690: 1687: 1686: 1682: 1680:408 MHz 1679: 1676: 1672: 1668: 1665: 1663: 1660: 1659: 1655: 1653: 1651: 1647: 1643: 1640: 1637: 1636: 1633: 1629: 1627: 1624: 1620: 1617: 1614: 1613: 1609: 1607: 1604: 1600: 1596: 1593: 1591: 1590:Yebes RT 40 m 1588: 1587: 1583: 1581: 1578: 1577:Moscow Oblast 1575: 1572: 1568: 1567: 1563: 1560: 1557: 1554: 1553: 1550: 1547: 1544: 1541: 1539: 1535: 1534: 1530: 1526: 1524: 1521: 1518: 1515: 1514: 1510: 1505: 1503: 1500: 1497: 1494: 1493: 1489: 1484: 1482: 1479: 1476: 1473: 1472: 1468: 1465: 1462: 1459: 1456: 1453: 1452: 1448: 1445: 1442: 1439: 1436: 1433: 1432: 1428: 1425: 1422: 1419: 1417: 1414: 1413: 1409: 1406: 1403: 1401: 1397: 1393: 1391: 1388: 1387: 1383: 1381:0–2 GHz 1380: 1377: 1373: 1370: 1368: 1365: 1364: 1360: 1357: 1355: 1351: 1347: 1344: 1341: 1340: 1336: 1332: 1329: 1327: 1323: 1319: 1316: 1313: 1312: 1308: 1304: 1301: 1298: 1294: 1292: 1289: 1288: 1284: 1281: 1278: 1275: 1274: 1268: 1261: 1257: 1253: 1251: 1249: 1245: 1242: 1239: 1238: 1234: 1231: 1229: 1225: 1222: 1219: 1216: 1215: 1212: 1208: 1205: 1203: 1199: 1196: 1194: 1191: 1190: 1186: 1182: 1178: 1175: 1173: 1169: 1168:Coonabarabran 1165: 1162: 1159: 1158: 1154: 1150: 1146: 1143: 1140: 1136: 1132: 1129: 1126: 1123: 1122: 1119: 1115: 1112: 1110: 1106: 1103: 1100: 1099: 1095: 1092:on behalf of 1091: 1087: 1085: 1083: 1079: 1076: 1072: 1069: 1068: 1064: 1060: 1056: 1052: 1049: 1047: 1043: 1039: 1036: 1032: 1029: 1028: 1024: 1020: 1017: 1014: 1012: 1008: 1005: 1001: 998: 997: 993: 990: 987: 984: 983: 977: 970: 966: 962: 958: 954: 951: 948: 945: 944: 939: 936: 933: 930: 927: 926: 922: 919: 916: 913: 910: 908: 905: 904: 900: 896: 893: 890: 887: 885: 882: 881: 877: 873: 869: 865: 861: 857: 854: 851: 849: 846: 845: 841: 837: 834: 831: 828: 826: 823: 822: 818: 814: 811: 808: 804: 801: 799: 796: 795: 791: 788: 785: 782: 779: 776: 775: 771: 768: 765: 763: 759: 758:Suffa plateau 756: 754: 751: 750: 746: 743: 740: 737: 733: 730: 728: 725: 724: 720: 717: 714: 711: 710: 705: 703:5.7 GHz 702: 699: 696: 693: 692: 688: 684: 681: 678: 675: 673: 670: 669: 665: 662: 659: 656: 654: 651: 650: 646: 642: 638: 635: 632: 628: 625: 622: 619: 618: 614: 610: 606: 603: 600: 596: 593: 590: 587: 586: 582: 579: 576: 573: 572: 568: 565: 562: 559: 558: 554: 551: 549:Miyun, China 548: 545: 544: 540: 538:232 MHz 537: 535:Miyun, China 534: 531: 530: 525: 522: 519: 516: 515: 511: 508: 505: 502: 499: 498: 494: 490: 487: 484: 481: 480: 476: 473: 470: 468: 465: 464: 460: 456: 453: 450: 446: 443: 441: 438: 437: 433: 430: 427: 424: 423: 417: 410: 406: 402: 399: 397: 394: 391: 388: 387: 383: 379: 376: 374: 371: 368: 365: 364: 360: 357: 354: 351: 350: 344: 337: 333: 330: 327: 324: 321: 318: 317: 313: 309: 306: 303: 300: 298: 295: 294: 290: 287: 284: 281: 279: 276: 275: 271: 268: 266: 262: 258: 255: 252: 251: 247: 244: 241: 238: 235: 232: 231: 227: 224: 221: 218: 215: 212: 211: 208: 204: 200: 197: 194: 190: 187: 184: 183: 179: 176: 173: 169: 166: 163: 162: 158: 155: 152: 149: 146: 143: 142: 138: 134: 131: 128: 125: 123: 120: 119: 115: 112: 109: 106: 105: 99: 97: 94: 92: 88: 84: 80: 72: 67: 60: 55: 45: 36: 32: 29:This list is 27: 20: 19: 16: 7670:Solar System 7475:Astronomy by 7436:Arno Penzias 7376:Cyril Hazard 7018:South Africa 6809:(Uzbekistan) 6685: 6649:Radio window 6555: 6545: 6533:. Retrieved 6529:the original 6519: 6507:. Retrieved 6503: 6494: 6482:. Retrieved 6478:the original 6473: 6450:. Retrieved 6448:. 2020-12-01 6445: 6436: 6425:. Retrieved 6421:the original 6411: 6394: 6388: 6377:. Retrieved 6367: 6356: 6345:. Retrieved 6341:the original 6331: 6320:. Retrieved 6316: 6307: 6262: 6258: 6248: 6237:. Retrieved 6233: 6224: 6213:. Retrieved 6211:. APEX. 2018 6203: 6189: 6178:. Retrieved 6169: 6158:. Retrieved 6148: 6136:. Retrieved 6132: 6123: 6112: 6100:Ghostarchive 6098:Archived at 6094: 6082:. Retrieved 6078: 6069: 6057:. Retrieved 6053: 6044: 6032:. Retrieved 6028: 6019: 6008:. Retrieved 6004:the original 5994: 5982:. Retrieved 5978: 5969: 5957:. Retrieved 5953: 5944: 5932:. Retrieved 5928: 5919: 5907:. Retrieved 5904:Eaaro.org.uk 5903: 5879:. Retrieved 5875: 5849:. Retrieved 5846:Meteoriti.lv 5845: 5821:. Retrieved 5817: 5808: 5796:. Retrieved 5793:Lud.bmstu.ru 5792: 5783: 5758:. Retrieved 5751:the original 5738: 5726:. Retrieved 5722: 5682:. Retrieved 5678:the original 5653:. Retrieved 5649: 5640: 5631: 5622: 5613: 5604: 5595: 5586: 5572: 5558: 5544: 5530: 5518:. Retrieved 5513: 5504: 5471: 5461: 5449:. Retrieved 5444: 5435: 5424:. Retrieved 5420: 5411: 5400:. Retrieved 5396:the original 5386: 5375: 5363:. Retrieved 5359:the original 5349: 5324:. Retrieved 5317:the original 5304: 5292:. Retrieved 5288: 5279: 5270: 5261: 5250:. Retrieved 5246: 5237: 5225:. Retrieved 5221:the original 5216: 5207: 5195:. Retrieved 5191: 5179: 5167:. Retrieved 5163: 5154: 5142:. Retrieved 5138: 5129: 5117:. Retrieved 5113:the original 5108: 5099: 5085: 5074:. Retrieved 5070:the original 5060: 5048:. Retrieved 5044:the original 5030: 5018:. Retrieved 5008: 4997:. 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JRO. 2021 6317:Das.inpe.br 6138:14 December 6084:14 December 6079:Eracnet.org 6034:14 December 6029:Eracnet.org 5984:14 December 5959:14 December 5934:14 December 5909:14 December 5881:14 December 5876:Ira.inaf.it 5851:14 December 5823:14 December 5798:14 December 5728:14 December 5655:14 December 5365:14 December 5294:14 December 5227:14 December 5197:14 December 5169:14 December 4413:Space-based 4336:of Taiwan. 4193:Puerto Rico 4025: [ 3613:35-950 GHz 2481:San Basilio 2376:, Portugal 2123:Kirkkonummi 2097:Kilpisjärvi 1863:detectors. 1840:Pico Veleta 1823: [ 1630:RT4 (32 m) 1603:Guadalajara 1457:(TNA-1500) 1437:(TNA-1500) 1078:Tidbinbilla 1053:6x22m dish 969:Pyeongchang 965:Jeju Island 832:, Thailand 609:wavelengths 599:Maharashtra 7680:Categories 7477:EM methods 6697:telescopes 6695:Individual 6484:25 October 6452:2020-12-02 6427:2008-08-26 6379:2021-02-14 6347:2010-01-28 6322:2010-01-28 6272:2107.01633 6239:2019-11-10 6215:2020-06-21 6180:2020-09-02 6160:2020-11-25 6059:18 January 6010:2013-05-10 5872:"IRA Home" 5760:2017-07-07 5684:2008-08-14 5426:2021-09-21 5402:2019-06-23 5326:2017-07-07 5252:2007-01-23 5076:2007-01-23 4999:2007-01-23 4937:References 4566:, England 3988:Cassegrain 3977:(CASLEO), 3876:(NANTEN2) 3690:micromesh 3436:New Mexico 3416:. 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Index

incomplete
adding missing items

Atacama Large Millimeter Array

Ukrainian T-shaped Radio telescope, second modification
radio astronomy
dishes
interferometric
AVN-Ghana
Kuntunse
VLBI
C-BASS
Meerkat National Park
Hartebeesthoek Radio Astronomy Observatory
Johannesburg
Hartebeesthoek Radio Astronomy Observatory
Johannesburg
MeerKAT
Hydrogen Epoch of Reionization Array
Meerkat National Park
Hydrogen Intensity and Real-time Analysis eXperiment
Meerkat National Park
Durban University of Technology
Durban
South Africa
KAT-7
Meerkat National Park
MeerKAT
Meerkat National Park

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