• Skip to main content
  • Skip to primary sidebar
  • Skip to footer

Dark Energy Spectroscopic Instrument (DESI)

  • / science /
    • science overview
    • cosmology and dark energy
    • redshifts and distance
    • mapping the universe
    • the DESI science mission
    • the DESI survey
    • imaging surveys
  • / instrument /
    • instrument overview
    • telescope
      • tohono o’odham
    • corrector
    • focal plane system
    • fiber system
    • spectrograph
    • instrument control system
    • data systems
    • bringing DESI to life
      • commissioning Instrument
      • protoDESI
  • / collaboration /
    • DESI team
    • DESI builders
    • collaborating institutions
    • sponsors
    • code of conduct
    • vendors
    • collaboration policies
  • / press /
    • announcements
    • in the news
    • press releases
    • tweets by desisurvey
    • blog
    • acknowledgments
  • / galleries /
    • videos
    • image gallery
  • / for scientists /
    • data releases
    • instrument design
    • imaging data
    • target selection and survey validation
    • theory and simulations
    • other DESI science
    • key publications
    • all DESI papers
    • team login
    • request a DESI speaker
    • internal
  • / education & outreach /
    • meet a DESI member
    • blog
    • planetarium show
    • DESI high
    • interactive visualizations
    • DESI Merch

protoDESI

Spectrograph

The ProtoDESI experiment was designed to answer the question: Can DESI align its optical fibers with the targets using robotic positioners, and keep them aligned for the duration of a DESI exposure?

The answer: Yes. ProtoDESI demonstrated the successful performance of the robotic positioners and alignment system.

ProtoDESI is a subset of DESI subsystems. It was built to operate with a simplified prime focus instrument, a Fiber View Camera (FVC) for positioning feedback, Telescope Control System (TCS), and Instrument Control System (ICS). Rather than measuring the output of a 50-meter fiber cable with DESI’a spectrographs, ProtoDESI confirmed fiber pointing and stability with a fiber photometry camera (FPC) that imaged the ends of the short 3-meter fibers mounted on the prime focus instrument. The success of ProtoDESI relied heavily on the interaction of its hardware and software, and on the careful translation between focal plane coordinates and target locations. ProtoDESI was mounted to the Mayall telescope from August 15 to September 30, 2016.

A photo of DESI researchers taken after the first successful alignment of ProtoDESI fibers with targets
ProtoDESI installed in the prime focus of the Mayall Telescope

Primary Sidebar

  • instrument overview
  • telescope
    • tohono o’odham
  • corrector
  • focal plane system
  • fiber system
  • spectrograph
  • instrument control system
  • data systems
  • bringing DESI to life
    • commissioning instrument
    • protoDESI

Footer

TEAM LOGIN

twitter   instagram   facebook

Copyright © 2018 Dark Energy Spectroscopic Instrument [DESI]

Copyright © 2025 · Parallax Pro DESI on Genesis Framework · WordPress · Log in