Processing and analyzing hundreds of terabytes of data can take longer than researchers would like. Today’s authors use the power of citizen science to find 142 new flickering sources of radio emission!
The second white dwarf pulsar ever discovered was just announced, and it can teach us a lot about how these unique stars evolve!
Today’s authors find that the host galaxy of the brightest gamma-ray burst ever detected is unexpectedly average!
We can’t exactly put massive neutron stars on scales, so how do we measure their masses? Today’s paper introduces a new method, using high-energy gamma rays!
The optical pulses from a very special pulsar are showing up around 200 microseconds late- today’s authors investigate this very tiny lag to learn why!