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  2. Illustris project - Wikipedia

    en.wikipedia.org/wiki/Illustris_project

    The Illustris project is an ongoing series of astrophysical simulations run by an international collaboration of scientists. [1] The aim is to study the processes of galaxy formation and evolution in the universe with a comprehensive physical model.

  3. Hubble Ultra-Deep Field - Wikipedia

    en.wikipedia.org/wiki/Hubble_Ultra-Deep_Field

    The Hubble Ultra-Deep Field (HUDF) is a deep-field image of a small region of space in the constellation Fornax, containing an estimated 10,000 galaxies.The original data for the image was collected by the Hubble Space Telescope from September 2003 to January 2004 and the first version of the image was released on March 9, 2004. [1]

  4. Hubble Deep Field - Wikipedia

    en.wikipedia.org/wiki/Hubble_Deep_Field

    The dramatic improvement in Hubble's imaging capabilities after corrective optics were installed encouraged attempts to obtain very deep images of distant galaxies.. One of the key aims of the astronomers who designed the Hubble Space Telescope was to use its high optical resolution to study distant galaxies to a level of detail that was not possible from the ground.

  5. New telescope reveals stunning images of the universe as it ...

    www.aol.com/telescope-reveals-stunning-images...

    Pictures could also help tell some of the universe’s biggest secrets

  6. New celestial images will create a 3D map of the universe - AOL

    www.aol.com/celestial-images-create-3d-map...

    The first five images captured by the Euclid telescope showcase glimmering clusters of galaxies and stars. The telescope, launched in July, was designed to create the most detailed 3D map of the ...

  7. List of deep fields - Wikipedia

    en.wikipedia.org/wiki/List_of_Deep_Fields

    In astronomy, a deep field is an image of a portion of the sky taken with a very long exposure time, in order to detect and study faint objects. The depth of the field refers to the apparent magnitude or the flux of the faintest objects that can be detected in the image. [2]