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  2. Transient Array Radio Telescope - Wikipedia

    en.wikipedia.org/.../Transient_Array_Radio_Telescope

    The Transient Array Radio Telescope (TART) is a low-cost open-source array radio telescope consisting of 24 all-sky GNSS receivers operating at the L1-band (1.575 GHz). TART was designed as an all-sky survey instrument for detecting radio bursts, as well as providing a test-bed for the development of new synthesis imaging and calibration ...

  3. GOTO (telescope array) - Wikipedia

    en.wikipedia.org/wiki/GOTO_(telescope_array)

    The Gravitational-wave Optical Transient Observer (GOTO) is an array of robotic optical telescopes optimized for the discovery of optical counterparts to gravitational wave events [1] and other multi-messenger signals. The array consists of a network of telescope systems, with each system consisting of eight 0.4m telescopes on a single mounting ...

  4. List of radio telescopes - Wikipedia

    en.wikipedia.org/wiki/List_of_radio_telescopes

    32m RT-32 radio telescope, operating range 1.4–22 GHz. [permanent dead link ‍] Svetloe Radio Astronomical Observatory Svetloe, Karelia, Russia 1.4–22 GHz 32m RT-32 radio telescope, operating range 1.4–22 GHz. [34] RT-7.5 (Bauman's radio telescope) Moscow Oblast, Russia Two 7.75-meter diameter antennas (only one is working at the moment ...

  5. High Energy Transient Explorer 1 - Wikipedia

    en.wikipedia.org/wiki/High_Energy_Transient...

    The HETE-1 satellite was launched with the Argentina satellite SAC-B. HETE-1 was lost during the launch on 4 November 1996, at 17:08:56 UTC, from Wallops Flight Facility (WFF), launch area-3. The Pegasus XL launch vehicle achieved a good orbit, but explosive bolts releasing HETE-1 from another satellite, SAC-B, and from its Dual Payload Attach ...

  6. Very Small Array - Wikipedia

    en.wikipedia.org/wiki/Very_Small_Array

    The Very Small Array (VSA) was a 14-element interferometric radio telescope operating between 26 and 36 GHz that is used to study the cosmic microwave background radiation. It was a collaboration between the University of Cambridge , University of Manchester and the Instituto de Astrofisica de Canarias ( Tenerife ), and was located at the ...

  7. Focal-plane array (radio astronomy) - Wikipedia

    en.wikipedia.org/wiki/Focal-plane_array_(radio...

    Traditional radio-telescopes have only one receiver at the focus of the telescope, but radio-telescopes are now starting to be equipped with focal plane arrays, which are of three different types: multi-beam feed arrays, bolometer arrays, and the experimental phased-array feeds.

  8. Zwicky Transient Facility - Wikipedia

    en.wikipedia.org/wiki/Zwicky_Transient_Facility

    The Zwicky Transient Facility (ZTF, obs. code: I41) is a wide-field sky astronomical survey using a new camera attached to the Samuel Oschin Telescope at Palomar Observatory in San Diego County, California, United States. Commissioned in 2018, it supersedes the (Intermediate) Palomar Transient Factory (2009–2017) that used the same ...

  9. 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 ...