FIES is a cross-dispersed high-resolution echelle spectrograph with a maximum spectral resolution of R = 67000. The entire spectral range 370-830 nm is covered...
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InstallationHigh-resolution FIbre-fed Echelle Spectrograph
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InstallationHIPERCAM
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InstallationIntermediate Dispersion Spectrograph
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...
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InstallationIO-O
IO:O was originally equipped with a Fairchild 486 CCD detector. However, this was found to have degraded during storage resulting in poor blue Quantum...
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InstallationIsaac Newton Telescope
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...
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InstallationLARS
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InstallationLCO's Network of Robotic Echelle Spectrographs
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...
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InstallationLiverpool Telescope
The Liverpool Telescope is a 2 metre diameter optical astronomical telescope, constructed especially for robotic use. The telescope is especially to study...
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InstallationLong-slit Intermediate Resolution Infrared Spectrograph