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The Dark Energy Spectroscopic Instrument (DESI) has finished its originally planned five-year survey, producing the most detailed three-dimensional map of the universe to date.
Completed ahead of schedule on April 14–16, 2026 at Kitt Peak National Observatory in Arizona, DESI has recorded spectra for more than 47 million galaxies and quasars and over 20 million stars using 5,000 fiber-optic positioners on the Nicholas U. Mayall 4‑meter telescope.
Managed by Lawrence Berkeley National Laboratory, the international collaboration of roughly 900 researchers exceeded initial targets of 34 million objects and will continue observations and possible upgrades into the late 2020s.
The dataset—covering tens of thousands of square degrees and spanning billions of years of cosmic history—provides precise redshifts essential for baryon acoustic oscillation and other probes of cosmic expansion.
Early DESI results from year-one data hinted that dark energy may be evolving rather than constant; the full five-year survey will allow that signal to be tested.
Processing and validation of the full dataset are underway, with first papers based on the complete survey expected in 2027 and further public releases to follow.







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