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  2. Green Bank Observatory - Wikipedia

    en.wikipedia.org/wiki/Green_Bank_Observatory

    Green Bank Observatory is a location in Fallout 76, as National Isolated Radio Array [16]; The observatory is called Camp Echo One in “Captain America: Brave New World,” with Captain America entering a radio quiet zone in West Virginia where two telescopes resemble the 100-meter Green Bank Telescope.

  3. Timeline of telescopes, observatories, and observing technology

    en.wikipedia.org/wiki/Timeline_of_telescopes...

    1963 – Arecibo 300-meter radio telescope begins operation, located in Arecibo, Puerto Rico; 1964 – Martin Ryle's 1-mile (1.6 km) radio interferometer begins operation, located in Cambridge, England; 1965 – Owens Valley 40-meter radio telescope begins operation, located in Big Pine, California; 1967 – First VLBI images, with 183 km baseline

  4. Very-long-baseline interferometry - Wikipedia

    en.wikipedia.org/wiki/Very-long-baseline...

    Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. In VLBI a signal from an astronomical radio source, such as a quasar, is collected at multiple radio telescopes on Earth or in space. The distance between the radio telescopes is then calculated using the time difference between the ...

  5. Atacama Large Millimeter Array - Wikipedia

    en.wikipedia.org/wiki/Atacama_Large_Millimeter_Array

    The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile, which observe electromagnetic radiation at millimeter and submillimeter wavelengths.

  6. Closure phase - Wikipedia

    en.wikipedia.org/wiki/Closure_phase

    Three radio telescope receivers. A minimum of three antennas are required for closure phase measurements. In the simplest case, with three antennas in a line separated by the distances a 1 and a 2 shown in diagram at the right. The radio signals received are recorded onto magnetic tapes and sent to a laboratory such as the Very Long Baseline Array.

  7. Submillimeter Array - Wikipedia

    en.wikipedia.org/wiki/Submillimeter_Array

    The Submillimeter Array (SMA) consists of eight 6-meter (20 ft) diameter radio telescopes arranged as an interferometer for submillimeter wavelength observations. It is the first purpose-built submillimeter interferometer, constructed after successful interferometry experiments using the pre-existing 15-meter (49 ft) James Clerk Maxwell Telescope and 10.4-meter (34.1 ft) Caltech Submillimeter ...

  8. European VLBI Network - Wikipedia

    en.wikipedia.org/wiki/European_VLBI_Network

    The European VLBI Network (EVN) is a network of radio telescopes located primarily in Europe and Asia, with additional antennas in South Africa and Puerto Rico, which performs very high angular resolution observations of cosmic radio sources using very-long-baseline interferometry (VLBI). The EVN is the most sensitive VLBI array in the world ...

  9. Very Large Array - Wikipedia

    en.wikipedia.org/wiki/Very_Large_Array

    The VLA is a multi-purpose instrument designed to allow investigations of many astronomical objects, including radio galaxies, quasars, pulsars, supernova remnants, gamma-ray bursts, radio-emitting stars, the sun and planets, astrophysical masers, black holes, and the hydrogen gas that constitutes a large portion of the Milky Way galaxy as well ...