NanoFull is an ambitious interdisciplinary project to: i) understand the process of formation process of fullerene- and graphene-based molecular nanostructures in circumstellar envelopes through the decomposition of "natural" nanoparticles with aromatic and aliphatic composition; ii) detect other forms of carbon in space. Surprisingly, detections

The project aims at establishing a pipeline for the generation of galaxy mock catalogs using machine learning techniques. Such catalogs are key for the statistical analysis of forthcoming galaxy redshift surveys, some in which the IC is participating.

Using the publicly available cosmological fields of MUSE, we plan to detect the gas that feeds star formation in nearby galaxies. It would be the first time this gas is detected in Ha. The main advantage of using Ha with respect to Lya (used at high redshift) is the possibility of measuring metallicity and, thus, to be able to distinguish between

Four are the main objectives of this coordinated project, which are nevertheless synergistically related to one another. First, we must contribute to the tests until launch (February 2020) of SO/PHI aboard Solar Orbiter, and commission of the instrument for the three first years of flight (cruise phase of the mission), before the scientific

uno en el hemisferio norte y otro en el sur, que cubrirán todo el cielo. Pretende abarcar una sensibilidad y un rango de energías en el espectro electromagnético (entre decenas de Gigaelectronvoltios -GeV- y cientos de Teraelectronvoltios-TeV-); un orden de magnitud superior al de la generación de telescopios actual CTA permitirá desarrollar por

SOLARNET aimet at integrating all pertinent European research institutions, infrastructures, and data repositories in the field of high-resolution solar physics with the aim of: (i) realise transnational access to all European users; (ii) integrate small communities and foster European collaboration; (iii) enhance and spread data acquisition and