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...