
Dark Energy Spectroscopic Instrument
Instrument for conducting a spectrographic survey of distant galaxies

Instrument for conducting a spectrographic survey of distant galaxies
The Dark Energy Spectroscopic Instrument (DESI) is a scientific research instrument for conducting spectrographic astronomical surveys of distant galaxies. Its main components are a focal plane containing 5,000 fiber-positioning robots, and a bank of spectrographs which are fed by the fibers. The instrument enables an experiment to probe the expansion history of the universe and the mysterious physics of dark energy. The main DESI survey started in May 2021. DESI sits at an elevation of 6,880 feet (2,100 m), where it has been retrofitted onto the Mayall Telescope on top of Kitt Peak in the Sonoran Desert, which is located 55 miles (89 km) from Tucson, Arizona, United States. In March 2025, the DESI collaboration released Data Release 1 (DR1), containing spectra and redshifts for 18.7 million objects observed during the first 13 months of the main survey, making it the largest spectroscopic redshift dataset released at the time. Analysis of DESI's first three years of cosmological data,...
Read on Wikipedia · Image Lawrence Berkeley National Lab/KPNO/NOIRLab/NSF/AURA, CC BY 4.0
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