The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
Abstract We describe the spectroscopic data processing pipeline of the Dark Energy Spectroscopic Instrument (DESI), which is conducting a redshift survey of about 40 million galaxies and quasars using a purpose-built instrument on the 4 m Mayall Telescope at Kitt Peak National Observatory. The main goal of DESI is to …