The Sun is well known for its magnetic activity, including periodic flares that rise from its surface when magnetic field lines tangle, cross or reorganise near sunspots. Flares send streams of charged particles into space. If they are directed towards Earth, these particles can disrupt satellites or cause colourful auroral displays. The EU-funded

X-ray binaries are excellent laboratories to study the physics of relativistic stars. On the one hand, they provide robust evidence for the existence of black holes (BHs), the pinnacle of extreme gravity. On the other, they allow investigations on neutron stars (NS) the densest form of matter known. In addition, accretion on matter (provided by the

The EU-funded GALSIZE project aims to I) establish a new paradigm of galaxy data-model comparisons, II) characterize the nature of, and coupling between, dark and luminous matter in galaxies, with the aid of scaling relations, mass tracers, and numerical simulations, and III) expand model inferences into the uncharted realm of low-mass galaxies. To

Ramón y Cajal contract to develop his research work in the specific research project Galaxy Formation in the Big-Ddata Era

Our novel project principally comprises mobilities which form the backbone of a programme for educating new leaders in astronomical research through international collaboration across old and new EU member states. This new project will make use of our previous successful partnership "Per Aspera Ad Astra Simul" which initiated these collaborations

Contract Ramón y Cajal to develop his research work in the specific research project "Weak decays of hadrons as laboratories of New Physics and QCD".