Instruments by Type

Wide Field Direct Optical/IR Spectrographs
  • Binospec for MMT
  • DEIMOS for Keck
  • IMACS
  • NIRMOS for VLT
  • VIMOS for VLT
    • Fiber Fed Optical Spectrographs
  • Echidna for Subaru
  • FLAMES for VLT
  • Hectospec for MMT
  • Hectochelle for MMT
  • Lick AMOS
  • Hydra CTIO
  • Hydra WIYN
  • MIKE for Magellan
  • 2dF for AAT
  • 6dF for UK Schmidt
  • WHT Autofib2
    • High Dispersion Optical Spectrographs
  • ESI for Keck
  • HDS for Subaru
  • Hectochelle for MMT
  • HIRES for Keck
  • HROS for Gemini
  • HRS for Hobby-Eberly
  • MIKE for Magellan
  • UVES for VLT
    • Very Wide Field Optical-IR Cameras
  • MMT Megacam
  • CFHT MegaPrime
  • Sloan Digital Sky Survey
  • Suprime-Cam for Subaru
  • ESO'S VST with Omegacam (2.6m to support VLT)
  • UK's VISTA (4m with optical/IR cameras)
    • Near IR Spectrographs
  • CIRPASS for Gemini
  • CRIRES for VLT
  • EMIR for GTC
  • FLAMINGOS
  • Gemini Near IR Spectrograph
  • IRCS for Subaru
  • ISAAC for VLT
  • LUCIFER for LBT
  • NIRI for Gemini
  • NIRSPEC for Keck
  • Phoenix for Gemini
  • SINFONI for VLT
    • Near IR Cameras
  • CONICA for VLT
  • EMIR for GTC
  • FLAMINGOS
  • Hokupa'a/QUIRC for Gemini
  • IRCS for Subaru
  • ISAAC for VLT
  • LUCIFER for LBT
  • NIRC for Keck
  • NIRC2 for Keck
  • NIRI for Gemini
    • Adaptive Optics Systems
  • Tutorial on Adaptive Optics - Imperial College
  • Center for Adaptive Optics (NSF-Lick)
  • Center for Astronomical Adaptive Optics (UofA)
  • ESO Adaptive Optics
  • Gemini Adaptive Optics
  • Keck Adaptive Optics
  • Livermore Laser Guide Star Adaptive Optics
  • University of Hawaii Adaptive Optics
    • Back to Home Page