NIRPS is a next-generation, near-infrared spectrograph that uses adaptive optics and is fed via a fiber link. It is a compact cryogenic Echelle spectrograph...

The Near Infrared Spectrometer and Photometer (NISP) is an infrared spectrograph for the EUCLID mission. The aim of EUCLID is to obtain a map of the Dark matter...

A project for the technological demonstration of the use of FPGAs (Field Programmable Gate Array) in the field of adaptive optics systems.

Optical communication operations with the OGS. The aim of this project is to characterise optical communications from the earth to artificial satellites.

Participation in OPTICON. One of the main goals of this project, to which many of the individual activities being carried out at OPTICON are also contributing...

OSIRIS is a camera and intermediate spectrograph in operation in the GTC telescope. OSIRIS has various observation modes: direct image, wide slit and multi-slit...

PLAnetary Transits and Oscillations of stars (PLATO) is the third medium-class mission in ESA's Cosmic Vision programme. Its objective is to find and study a...

A Cosmic Microwave Background Polarimeter

QUIJOTE (Q-U-I JOint TEnerife CMB experiment) - is a program with two telescopes and a battery of instruments, installed in the Teide Observatory, dedicated to...