Post-detection of a gravitational wave background, pulsar timing arrays could detect individual sources of gravitational waves, called Continuous Waves. Let’s find out what properties we expect them to have!
How did supermassive black holes grow in the early universe? Finding faint and distant AGN with JWST may help us unravel this mystery!
The upcoming LISA mission promises to detect many gravitational wave events, but can it attribute any of them to a host galaxy? Let’s find out!
In this Astrobite, we look at black hole mergers in the accretion disks around supermassive black holes, because you can simply never have too many black holes!
A recent observation of an extremely distant quasar sheds some (X-ray) light on the long-standing mystery of supermassive black hole formation.
In a magical act some stars could vanish from the night sky, today’s bite asks: can we can see them again as black holes?