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

Grants for the training of doctors in Severo Ochoa Research Centers and Centers of Excellence

The Transiting Exoplanet Survey Satellite (TESS) is a NASA mission that started scientific operations in July 2018. Over two years it will cover the entire sky, searching for planetary transits in stars with magnitudes brighter than 14. Data covering the first 3 weeks of the mission were released in September 2018, and within days a super-earth