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Some of the Atacama Large Millimeter Array radio telescopes The eight radio telescopes of the Smithsonian Submillimeter Array, located at the Mauna Kea Observatory in Hawai'i VLBI was used to create the first image of a black hole, imaged by the Event Horizon Telescope and published in April 2019. [1] Very-long-baseline interferometry (VLBI) is ...
Package Name Pro. Am. Interface Connects to Online (e.g. VO) Data Displays or Manip. FITS Images Tiled Multi-Resolution All-Sky image Handling Displays
WorldWide Telescope (WWT) is an open-source set of applications, data and cloud services, [4] [5] originally created by Microsoft Research but now an open source project hosted on GitHub. [6] The .NET Foundation holds the copyright and the project is managed by the American Astronomical Society and has been supported by grants from the Moore ...
A refracting telescope (also called a refractor) is a type of optical telescope that uses a lens as its objective to form an image (also referred to a dioptric telescope). The refracting telescope design was originally used in spyglasses and astronomical telescopes but is also used for long-focus camera lenses .
These lenses, and the telescope's filters, are built into the camera assembly. The first lens, at 1.55 m in diameter, is the largest lens ever built, [39] and the third lens forms the vacuum window in front of the focal plane. [38] Unlike many telescopes, [40] the Rubin Observatory makes no attempt to compensate for dispersion in the atmosphere ...
FOCAL (an acronym for Fast Outgoing Cyclopean Astronomical Lens) is a proposed space telescope that would use the Sun as a gravity lens.The gravitational lens effect was first derived by Albert Einstein, [1] and the concept of a mission to the solar gravitational lens was first suggested by professor Von Eshleman, [2] and analyzed further by Italian astronomer Claudio Maccone [3] and others.
The telescope used by Berkowski was attached to 6 + 1 ⁄ 2-inch (17 cm) Königsberg heliometer and had an aperture of only 2.4 in (6.1 cm), and a focal length of 32 in (81 cm). Commencing immediately after the beginning of totality, Berkowski exposed a daguerreotype plate for 84 seconds in the focus of the telescope, and on developing an image ...
The observatory is a 1-meter Coudé telescope with a field of view of 0.7 degrees, supported by an English cross-axial mount inside a dome 12.5-meters in diameter. Its main purposes are: to be the optical ground station of the Artemis telecommunications satellite (the project from which the telescope takes its name)
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