Integral-field spectroscopic facility deployed at the Nasmyth focus of the WHT This instrument is particularly useful for kinematic studies of galaxies.

The Intermediate Dispersion Spectrograph (IDS) is a long-slit spectrograph which sits at the Cassegrain Focal station of the 2.5m Isaac Newton Telescope and is...

The Isaac Newton Telescope (INT) has a 2.54-metre primary mirror with a focal ratio of f/2.94. It uses a polar-disc/fork type of equatorial mount. Instruments...

LCO's Network of Robotic Echelle Spectrographs (NRES) will be six identical high-resolution (R~53,000), precise (≤ 3 m/s), optical (380-860 nm) echelle...

The Liverpool Telescope is a 2 metre diameter optical astronomical telescope, constructed especially for robotic use. The telescope is especially to study...

LOTUS ( LO w-cos T U ltraviolet S pectrograph) is a low resolution optical-near UV spectrograph. The design is very simple, with no moving parts. It provides...

MAIA, the Mercator Advanced Imager for Asteroseismology is a new fast 3-channel photometric instrument MAIA, an acronym for Mercator Advanced Imager for...

Full disk resonant scattering spectrometer providing radial velocity measurements of the Sun at the Potassium KI 769.9 nm line. It belongs to the HIROS (High...