Today’s guest post by Joshua Lee discusses how one group used TESS asteroseismology to better characterize a star and its planet.
History has been made! The first magnetic field inside a main-sequence star has been measured!
Authors of today’s paper combine powerful machine learning techniques and millions of light curves to create the first all-sky galaxy mass map.
Do stars really spin down? Authors of today’s paper find out if what we’re seeing is real or a trick of the light.
Happy Red’s release week, swifties! Today we discuss a paper about RED giants, and how you can tell if they had undergone a merger or not!
In the latest of our #UndergradResearch series, discover how Larissa Palethorpe finds a way to get more information out of transit light curves.