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First light
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In astronomy, first light is when a telescope (or, in general, a new instrument) is first used to take an astronomical image after it has been constructed. This is not often the first viewing using the telescope; optical tests have likely already been performed during daylight to adjust the components.

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Encyclopedia
In astronomy, first light is when a telescope (or, in general, a new instrument) is first used to take an astronomical image after it has been constructed. This is not often the first viewing using the telescope; optical tests have likely already been performed during daylight to adjust the components. The first light image is normally of little scientific interest and is of poor quality since the various telescope elements must be adjusted for optimum efficiency. Usually, a well-known and spectacular astronomical object is chosen. Despite this, a first light is always a moment of great excitement, both for the people who designed and built the telescope, and for the astronomical community.
For example, the then-new 200-inch Hale saw first light January 26, 1949, targeting NGC 2261. under the direction of American astronomer Edwin Powell Hubble, which was published in many magazines.
The largest binocular telescope, the largest optical reflecting telescope in many areas, the Large Binocular Telescope, had its first light with a single primary mirror on October 12, 2005 which viewed NGC 891. The second primary mirror was installed in January 2006 and became fully operational in January 2008.
In cosmology, first light refers to the light emission from the first generation of stars, formed less than a billion years after the big bang.
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