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...

IO:I is the near-infrared imaging component of the IO suite of instruments. It uses a 2048x2048 pixel Hawaii 2RG 1.7μm cutoff detector with a field of view of 6...

Observing modes: Long-slit spectroscopy; Spectro and Imaging Polarimetry; Fast Spectroscopy; Image-slicer

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...

Retirado en 2022 para dar paso a nuevas instalaciones.

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...

Espectrógrafo infrarrojo de alta resolución para el Gran Telescopio de Canarias (GTC) del Observatorio del Roque de los Muchachos en la isla de La Palma. El...