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.
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.
The LBT f/15 Rigid Secondary Mirror enabled the LBT's MODS and LUCI facility instruments to get on sky before the adaptive secondary mirrors arrived.
KELT, OSU's first fully-robotic telescope, eventually discovered 26 transiting exoplanets around bright stars.