B-CycleS is born as an ambitious long-term research program that aims to provide a comprehensive picture for the formation and evolution of galaxies by studying...
The formation of fullerene molecular nanostructures in space
NanoFullerenes is an ambitious interdisciplinary project to understand the top-down formation process of fullerene molecular nanostructures in space, involving...
The internal structure of ionized nebulae and its effect on determining the chemical composition of the interstellar medium and the Universe
The project focuses on the study of the effect of the internal structure of temperature and density in ionized nebulae on the determination of their chemical...
The LiteBIRD space mission: development of the thermal monitoring and control system and scientific preparation
The main goal of this project is to guarantee and strengthen the technological and scientific contributions of the IAC to LiteBIRD, a JAXAled space mission...
The structure and evolution of galaxies and their outskirts
We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes...
Tracing galaxy evolution with nuclear structures in late-type galaxies - PROJECT 101108180 — TRANSLATE
Central regions of galaxies are inhabited by dense small structures, such as nuclear star clusters (NSCs) and nuclear disks and rings. These, at the bottom of...
Tracking active galactic nuclei feedback from parsec to kiloparsec scales
Active galactic nuclei (AGN) feedback is the effect that nuclear activity produces in the interstellar and circumgalactic medium (ISM and CGM) of galaxies...
Unravelling the dark universe from the Canary Island observatories - UNDARK
Astrophysical and cosmological observations imply that only 5% of the energy of the Universe is made of conventional matter. The rest is composed by a new type...
UNVEILING THE COMPLEXITY OF RADIO FOREGROUNDS FOR THE DETECTABILITY OF THE CMB POLARIZATION B-MODE
The aim of RadioForegroundsPlus is to combine the nine Planck all-sky (30-857 GHz) maps, with three unique low-frequency data sets: the QUIJOTE maps (at 11, 13...