Molecular Gas and Dust in Galaxies Across Cosmic Time
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...
This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way...
MOSAIC-S3T: Enhancing the S3T Ground Segment through Coordinated Multi-Sensor Observation using Stare and Chase Techniques and Data Fusion Analysis
The main goal of MOSAIC-S3T project (Enhancing the S3T Ground Segment through Coordinated Multi-Sensor Observation using Stare and Chase Techniques and Data...
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...
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...
Nuclear Activity in Galaxies: a 3D Perspective from the Nucleus to the Outskirts
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...
Nucleosynthesis and molecular processes in the late stages of Stellar Evolution
Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch...
The LPIYA Group gathers communicators and representatives from every institution present at the Roque de los Muchachos Observatory (ORM), with the objective of...