The new paradigm of the space sector, with a drastic reduction in launch costs and the rise of small satellites, demands more than ever the introduction of innovative technologies, especially in a sector as emerging today as the Earth Observation market.Within this framework, the IACTEC-Space group of the Instituto de Astrofísica de Canarias

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

The last decade has witnessed the beginning of the experimental program in the Large Hadron Collider (LHC) at CERN that early on, in 2012, reached one of its major milestones with the discovery of the Higgs. This favors a simple mechanism for the electroweak symmetry breaking (EWSB) which, combined with the absence of other new particles, confirms

The Sun, our star, is not only the source of the electromagnetic radiation that bathes our planet; it also sweeps the Earth's magnetosphere with its wind and heliospheric magnetic field. It frequently sends huge ropes of magnetized plasma, the coronal mass ejections, that can hit us and cause solar storms, thus constituting a serious potential

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