The general aim of the project is to research the structure, evolutionary history and formation of galaxies through the study of their resolved stellar populations, both from photometry and

This project studies the physical and compositional properties of the so-called minor bodies of the Solar System, that includes asteroids, icy objects, and comets. Of special interest are the trans

MIRADAS is an intermediate resolution infrared spectrograph for the GTC telescope. It will operate in the infrared range of 1 to 2.5 microns with a spectral resolution of 20,000. It is a multi-object spectrograph capable of observing up to 20 objects simultaneously, by means of a robot with 20 arms that can patrol a 5 arcminutes field.

Two of the most fundamental questions in astrophysics are the conversion of molecular gas into stars and how this physical process is a function of environments on all scales, ranging from planetary

This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way pretends to provide a data base for the

IAC is developing a Multi-Conjugate Adaptive Optics (MCAO) bench, with the purpose of demonstrating in laboratory solutions of some of the main problems related with solar MCAO to be applied to the

Infrared high-resolution echelle spectrograph for the Great Telescope CANARIAS (GTC) of the Observatorio del Roque de los Muchachos in the island of La Palma. The main scientific objective of the instrument is to measure the radial velocity (RV) with very high precision (goal of 1 m/s) in the near infrared.

The Carlos Sánchez and IAC80 telescopes, known as TTNN and located in the Teide Observatory, are telescopes manually operated by astronomers (in person or remotely) through specific computer

It is an initiative of the Instituto de Astrofísica de Canarias (IAC) via its Unit for Communication and Scientific Culture (UC3) with the collaboration of the scientific institutions of the Canary

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, capable of operating alone or in combination with the HARPS instrument. It will have a spectral resolution of 100000 or 75000, and will be installed in La Silla observatory (Chile).

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 of the Universe. NISP will provide near infrared photometry, low resolution spectra and redshifts of millions galaxies. IAC participates in the development of NISP Instrument Control Unit.

This project consists of two main research lines. First, the study of quasar-driven outflows in luminous and nearby obscured active galactic nuclei (AGN) and the impact that they have on their massive