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The Dark Energy Spectroscopic Instrument (DESI) collaboration has released the largest high-resolution three-dimensional map of the universe, built from a five-year observing campaign that recorded spectra from more than 47 million galaxies and quasars and over 20 million Milky Way stars.
Mounted on the 4-meter Nicholas U. Mayall Telescope at Kitt Peak, DESI uses 5,000 robotic fiber-optic positioners that reconfigure roughly every 20 minutes to feed ten spectrographs, achieving positional precision near 10 microns.
The survey exceeded its original 34âmillion target, completed final observations in April 2026 and involves over 900 researchers across more than 70 institutions.
By combining positions and distance measurements the map traces the cosmic web across 11 billion years of history and is being used to probe dark energyâs influence on cosmic expansion.
Early DESI data hinted dark energy may evolve with time; the full five-year dataset is under processing with definitive results expected in 2027.
DESI will continue observations through 2028 to expand sky coverage by roughly 20 percent and to refine measurements in crowded Milky Way and southern-sky regions.








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