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

We have a unique opportunity to make a definitive step forward and conclusively reconstruct the life of a typical (super) Milky-Way galaxy, from its initial clumpy gas-rich phase to its (inevitable?) death through quenching. Astronomy is indeed entering the big data era. Big-data spectro-photometric surveys such as LSST, EUCLID, WFIRST, JWST will

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

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