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Powerful telescope near me9/7/2023 ![]() A 40m single-dish short-millimetre telescope, operated by the National Astronomical Research Institute of Thailand (NARIT). Will be operated by XAO ( Xinjiang Astronomical Observatory).Ĭonstruction work started in 2017. RT-70, the construction started in 1981 but was never completed.įive hundred meter Aperture Spherical Telescope (FAST)ĥ00m radio telescope, the world's largest filled-aperture radio telescope, operating range 70–3000 MHz. RT-70, 70 m telescope, operating range 5–300 GHz ģ2 m RT-32 radio telescope, operating range 1.4–22 GHz. The SSRT is a special-purpose solar radio telescope designed for studying solar activity in the microwave range (5.7 GHz). 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. A Radioheliograph.Ī 45 m single-dish short-millimetre telescope, and six 10 m telescopes of the Nobeyama Millimetre Array (NMA), both operated by the National Astronomical Observatory of Japan (NAOJ) Operated by (Indian Institute of Astrophysics). ![]() Operated by the National Centre for Radio Astrophysics. Thirty 45 m wire dishes largest telescope at meter wavelengths. Operated by SHAO (Shanghai Astronomical Observatory) All of the 4.5m telescopes are assembled and the 2m telescopes will be assembled by 2013. CSRH will be used to study coronal mass ejections. CSRH will be one of the world's largest and most advanced imaging spectroscopy instruments. 40 telescopes of 4.5 m cover 400 MHz – 2 GHz and 60 telescopes of 2 m cover 2–15 GHz. The CSRH will consist of 100 telescopes covering 0.4–15 GHz. Construction started in 2004.ĬSRH is an interferometer under construction in China. PaST is planned to be an array of some ten-thousand log-periodic antennas spread over several square kilometers. Operated by XAO ( Xinjiang Astronomical Observatory). Operated by Purple Mountain Observatory.Ģ5 m. ġ0-m microwave telescope making observations of clusters using the Sunyaev-Zeldovich effect. Now disassembled, PAPER at its maximum had 128 crossed dipole antennas, making it the interferometer with more elements than any other at that time.ĭegree Angular Scale Interferometer (DASI)ġ3-element interferometer measuring anisotropies in the cosmic microwave background. Precision Array for Probing the Epoch of Reionization (PAPER) ![]() A pathfinder for the Square Kilometre Array. In progress – currently eight 6 m dishes with dual-polarization dipole antennas as feed at HartRAO.ĭurban University of Technology, Durban, South Africaĥ meter (16 foot) parabolic reflector Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) In progress – currently nineteen 14 m reflectors with crossed dipole antennas as feed. Hydrogen Epoch of Reionization Array (HERA) Hartebeesthoek Radio Astronomy Observatory, Johannesburg, South Africaġ5 m Experimental Demonstrator Model originally build as a technology demonstrator for MeerKAT The first radio telescope was invented in 1932, when Karl Jansky at Bell Telephone Laboratories observed radiation coming from the Milky Way.ģ2-metre (104 foot) single dish, first of African VLBI Network ħ.6-metre (24.9 foot) dish with polarimeter back end The list is sorted by region, then by name unnamed telescopes are in reverse size order at the end of the list. The list includes both single dishes and interferometric arrays. ![]() This is a list of radio telescopes – over one hundred – that are or have been used for radio astronomy. ( January 2021)įour of the sixty four total antennas of the ALMA radio telescope, at the Atacama Large Millimeter Array (ALMA) West arm of the low-frequency Ukrainian T-shaped Radio telescope, second modification (UTR-2) radio telescope phased array antenna This list is incomplete you can help by adding missing items. ![]()
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