The telescope attains median image quality 0.7 arcsec at 0.5 μm wavelength. Multiple instruments are available on standby, mounted at Nasmyth and bent-Cassegrain foci. Switching is accomplished within a few minutes by rotating the 45° tertiary mirror. This mirror is adjusted at high speed to prevent image blur from vibrations induced by wind-shake of the telescope structure.
Current (9/2007) instruments are
UV–optical 16-million pixel imager (SOI, CTIO)
near-infrared (1–2.4 μm wavelength) 1-million pixel HgCdTe imager and spectrograph (OSIRIS, Ohio State University/CTIO)
Additional instruments are scheduled to be commissioned in 2008 and 2009
UV–optical 16-million pixel imager and spectrograph (Goodman Spectrograph, UNC)
US astronomers access the telescope remotely over the Abilene Network. Chilean and Brazilian astronomers use their high-speed networks. An on-site operator controls where the telescope points while the remote astronomer controls the instrument and data retrieval.