A diffraction-limited high-resolution NIR spectrograph under development for the Large Binocular Telescope.
The Focal Plane System (FPS) units for SDSS-V replace the traditional Sloan Survey hand-plugged fiber plates with 500 robotic fiber positioners.
The Multi-Object Double Spectrographs (or MODS) are two facility UV-to-Near IR spectrographs for the Large Binocular Telescope.
The DESI Sky Continuum Monitor System tracks the night sky brightness to dynamically adjust exposure times to maximize DESI observing efficiency.
The DESI Commissioning Instrument jump-started commissioning of DESI by completing many critical on telescope tests before DESI was installed in 2019.
DEMONEXT was a 20-inch (0.5-m) robotic telescope designed for photometric monitoring of exoplanets and transient sources.
The three KMTNet prime focus CCD cameras are dedicated to gravitational microlensing searches for exoplanets on custom-designed 1.6m telescopes.
The Kitt Peak/CTIO Ohio State Multi-Object Spectrographs (K/COSMOS) are modified versions of the OSMOS spectrograph for the 4-m Mayall and Blanco telescopes.
The Ohio State Multi-Object Spectrograph (OSMOS) is the workhorse facility optical spectrograph at MDM.