The VO And Why It Matters To You In the most technical words, the Virtual Observatory (VO) is an effort to enable uniform and efficient access to astronomical data. With […]

Project 8 - towards a radio frequency measurement of the neutrino mass While neutrino flavour oscillations are a clear indication that neutrinos do have non-vanishing rest masses, their values have […]

The core of the matter – spatially resolving the nuclei of Active Galaxies with VLTI/GRAVITY One of the most exciting opportunities offered by the new VLT beam combiner GRAVITY is […]

Measuring the properties of cosmic rays with the radio technique The radio emission from air showers is now routinely detected to measure the properties of cosmic rays. An overview is […]

Axions from Sun? Exploring the low-energy frontier with the IAXO experiment Axions are ultralight hypothetical particles originally postulated to explain the observed smallness of the neutron´s electric dipole moment and […]

HAWC

Cosmic-ray acceleration - limits and laboratories I will review the current theoretical status of shock acceleration at supernova type shocks, with an emphasis on the plasma theory and implications for […]

The Crab nebula and pulsar - particle acceleration at the limit The Crab Nebula is the front-page object of multi-wavelength astrophysics and an excellent object to study non-thermal emission and […]

Up to two billion times acceleration of scientific simulations with deep neural architecture search Computer simulations are invaluable tools for scientific discovery. However, accurate simulations are often slow to execute, […]

Identifying sources of high-energy neutrinos of the AGN type: A theoretical approach Active galactic nuclei (AGN) have long been predicted to emit neutrinos if they host sites of cosmic-ray acceleration […]