International students were impacted in many ways during the pandemic. This paper attempts to study how they coped and what structural barriers they faced.
Pulsar timing arrays could localise individual sources of gravitational waves to host galaxies. The problem is, it’s so computationally difficult! This paper shows us a faster way.
![Garbage [priors] in, garbage [posteriors] out: The importance of astrophysics in tests of general relativity](https://i0.wp.com/astrobites.org/wp-content/uploads/2023/09/2002-12-12_Trou_noir-Black_hole.png?resize=320%2C260&ssl=1)
Before you fit your favourite models to some data, you should know something about your parameters beforehand! Find out why in today’s article
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!
We move through the universe relative to the Cosmic Microwave Background. Could our movement cause our measurements of the Hubble constant to be biased?
