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  2. MAXI (ISS experiment) - Wikipedia

    en.wikipedia.org/wiki/MAXI_(ISS_Experiment)

    The Monitor of All-sky X-ray Image (MAXI) is an X-ray telescope mounted on the International Space Station since 2009. The instrument uses wide field of view X-ray detectors to perform a sky survey , measuring the brightness of X-ray sources every 96 minutes (one ISS orbit).

  3. SPHEREx - Wikipedia

    en.wikipedia.org/wiki/SPHEREx

    SPHEREx will use a spectrophotometer to perform an all-sky survey that will measure near-infrared spectra from 0.75 to 5.0 micrometers. It will employ a single instrument with a single observing mode and no moving parts to map the entire sky (in 96 different color bands, far exceeding the color resolution of previous all-sky maps [4]) four times during its nominal 25-month mission; the crucial ...

  4. GOTO (telescope array) - Wikipedia

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

    The fast focal ratio of f/2.4 and large image sensor result in a relatively large field of view, with each GOTO system having a total FoV of approximately 40 square degrees, [2] around 200x the area of the full Moon in the sky. The fast focal ratio also means that only a small amount of time is needed to observe each area of the sky, with each ...

  5. Astronomical survey - Wikipedia

    en.wikipedia.org/wiki/Astronomical_survey

    GMRT - The Giant Metrewave Radio Telescope's TGSS ADR mapped the sky at 150 MHz. HTRU – A pulsar and radio transients survey of the northern and southern sky using the Parkes Radio Telescope and the Effelsberg telescope. Gamma-ray Fermi Gamma-ray Space Telescope, formerly referred to as the "Gamma-ray Large Area Space Telescope (GLAST)." 2008 ...

  6. Wide-field Infrared Survey Explorer - Wikipedia

    en.wikipedia.org/wiki/Wide-field_Infrared_Survey...

    In 2013, NASA reactivated the WISE telescope to search for near-Earth objects (NEO), such as comets and asteroids, that could collide with Earth. [12] [13] The reactivation mission was called Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE). [13] As of August 2023, NEOWISE was 40% through the 20th coverage of the full sky ...

  7. VLT Survey Telescope - Wikipedia

    en.wikipedia.org/wiki/VLT_Survey_Telescope

    The VLT Survey Telescope (VST) is a telescope located at ESO's Paranal Observatory in the Atacama Desert of northern Chile. It is housed in an enclosure immediately adjacent to the four Very Large Telescope (VLT) Unit Telescopes on the summit of Cerro Paranal. The VST is a wide-field survey telescope with a field of view twice as broad as the ...

  8. Pan-STARRS - Wikipedia

    en.wikipedia.org/wiki/Pan-STARRS

    The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS1; obs. code: F51 and Pan-STARRS2 obs. code: F52) located at Haleakala Observatory, Hawaii, US, consists of astronomical cameras, telescopes and a computing facility that is surveying the sky for moving or variable objects on a continual basis, and also producing accurate astrometry and photometry of already-detected objects.

  9. Keyhole problem - Wikipedia

    en.wikipedia.org/wiki/Keyhole_problem

    The green volume illustrates visible space limited by the keyhole problem. The arrow points to the "keyhole" as unviewable sky volume. To track celestial objects as they move across the sky, these systems usually rotate on two axes. Often, a tilting mechanism (elevation) is mounted upon a panning base . To cover the complete hemisphere of ...