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...

Future spectrograph with SGS autoguiding, adaptative optics system AO-L and CCD.

(Mid-resolution InfRAreD Astronomical Spectrograph) The infrared spectrograph of intermediate resolution, MIRADAS, will operate in the 1 to 2.5 micron infrared...

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...

Instrumento de espectroscopía 3D, MEGARA, se trasladará desde la Universidad Complutense de Madrid al GTC, donde se ha diseñado y construido en colaboración con...

MuSCAT2 is a new instrument offered at the Carlos Sanchez Telescope. It has been developed by the Astrobiology Center and the University of Tokyo (P.I. Norio...