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The Neil Gehrels Swift Observatory is a NASA spacecraft with telescopes designed to study gamma ray bursts—the most powerful explosions in the universe, which result from supernova explosions during the formation of neutron stars and black holes.

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The observatory was launched in 2004 as NASA's Swift Gamma-ray Observatory, but was renamed in 2018 in honor of the observatory's first principal investigator, Neil Gehrels, who passed away in 2017.
The observatory features the Burst Alert Telescope, which monitors up to 50% of the sky simultaneously for GRBs; an X-ray telescope that captures images of the GRB afterglow; and an ultraviolet/optical telescope to accurately locate GRBs and capture GRB afterglow information in these wavelengths.
Studying GRBs allows astronomers to better the formation of black holes, the formation of heavy elements, and the characteristics of the high-energy early universe.
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