Kachow! Three high energy neutrinos speed through IceCube
The IceCube collaboration presents the strongest limit yet on the proton fraction of ultra-high-energy cosmic rays.
The IceCube collaboration presents the strongest limit yet on the proton fraction of ultra-high-energy cosmic rays.
Today’s paper uses very deep JWST observations to hunt for some of the first galaxies ever formed!
Today’s authors find the highest energy neutrino *ever* with the up-and-coming KM3NeT neutrino observatory!
Segue 1 is one of the most diffuse galaxies we’ve ever detected. Is it the remnants of a larger galaxy? And can astronomers use it to understand dark matter?
Today’s authors investigate a few kinds of baby radio galaxies to learn about the life cycle of an active galactic nucleus!
Today’s paper summarizes various physical factors that can shape the duration of a GRB and propose that the duration of a GRB can be defined by four factors: progenitor, central engine, emitter, and geometry.