The European Solar Telescope (EST) (http://www.est-east.eu) is a European solar physics initiative involving more than 30 institutions from 18 countries, under the coordination of the IAC, representing the largest infrastructure of European research projected in the field of solar physics from Earth.

The NRT (New Robotic Telescope) is a project to design and build a 4-meter telescope within five years, which from the ORM will operate in a totally autonomous and robotic way. This form of operation will make it the largest robotic telescope in the world.

The CTAO is an initiative which is planning the construction of a new generation of Cherenkov Telescopes to study the universe in very high energy gamma-rays. Gamma-rays carry information about the most violent and extreme events in the universe.

The Free Space Optical Communications Group is focused in develop and research of quantum optical communications equipments and implementations,  between buildings, islands or with LEO/GEO satellite

Internal transversal research project that aims to bring together the know-how in machine learning and deep learning in the IAC. This project encapsulates the knowledge of machine learning in the

HARMONI is a first light optical / infrared spectrograph of integral field and high spatial resolution for ELT. Its design and construction is carried out by an international consortium in which the

High-resolution spectrograph for the 10-m Gran Telescopio Canarias (GTC) based on components from UES, a spectrograph which was in use at the 4.2-m William Herschel Telescope (WHT) between 1992 and 2001.

IAC participation in the HERSCHEL AND PLANCK SURVEYOR space missions. Since 1996 the Instituto de Astrofísica de Canarias has been a contributor to the concept and development processes for the scientific payload of the European Space Agency's (ESA) Herschel Space Observatory and Planck Surveyor missions.

The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars, 3) to search for extrasolar planets using

HARPS3 (High Accuracy Radial velocity Planet Searcher) is a new version of the succesful HARPS instrument. HARPS3 is an Echelle spectrograph with high resolution (R ~ 115000) and a wavelength range of 380-690 nm. It will be installed in the Isaac Newton Telescope (upgraded and robotized) at the ORM.

HARMONI is one of the three ELT (European Extremely Large Telescope) first light scientific instruments. It is a visible and near-infrared (0.47 to 2.45 µm) integral field spectrograph, providing the ELT's core spectroscopic capability, over a range of resolving powers from R (≡λ/Δλ) ~4000 to R~20000.

The Adaptive Optics (AO) for the Gran Telescopio Canarias (GTC) corrects the effect of the atmospheric turbulence on the light, to exploit the high spatial resolution capability of GTC. The Laser Guide Star (LGS) extends the coverage of GTCAO to any part of the sky, increasing dramatically the capability to do high spatial resolution science.