Line intensity mapping is an exciting new technique used to map the universe, but it struggles with astrophysical foregrounds. Today’s authors use the power of team work (data at other wavelengths) to make an intensity-mapping detection.
Today’s paper uses JWST to show that there are more spiral galaxies in the early universe than we previously expected.
Stellar radio emission is generally associated with active stars, but is it always? These authors investigate!
As we find more planetary systems, the question of “how unique is our solar system?” can begin to be put into context.
Learn about the “solar neutrino problem” and how it was solved!
In today’s post, guest author Zachary Pleska breaks down a recent study on the globular cluster NGC 419 and why some of its stars don’t evolve as expected!