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...
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InstallationLOw-cosT Ultraviolet Spectrograph
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InstallationMAIA
MAIA, the Mercator Advanced Imager for Asteroseismology is a new fast 3-channel photometric instrument MAIA, an acronym for Mercator Advanced Imager for...
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InstallationMark-I
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...
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InstallationMOSaic CAmera
MOSCA is a direct CCD camera mounted in the Cassegrain focus. The curvature of the focal plane is corrected by a field flattener window. Actually this is the...
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InstallationNordic Optical Telescope
The Nordic Optical Telescope (NOT) is a modern 2.6-m optical/IR telescope, located at the highest site of the Roque de los Muchachos Observatory. Inaugurated in...
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InstallationOSIRIS Nasmyth-B
It will be dismounted at the arrival of GTCAO in mid-2018, and will be moved to main Cassegrain station once available (estimated in mid-2019). 7.8 x 7.8 arcmin...
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InstallationPAUCam
PAUCam is an optical imaging camera to be used at the prime focus of the William Herschel Telescope (WHT). The camera covers 1 deg2 FoV with 18 Hamamatsu...
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InstallationRINGO3
RINGO3 is a fast-readout optical imaging polarimeter. It uses a polaroid that rotates once per second to measure the polarisation of light entering the...
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InstallationRISE
RISE is a fast-readout camera developed in collaboration with the Queens University Belfast for the precision measurement of transiting exoplanet timing. The...