I’m a cosmologist at the University of Cambridge.

I’m working on gravitational lensing, the phenomenon of massive objects deflecting light due to the local curvature they induce on spacetime. By observing gravitational lensing, we can learn about the distribution and behaviour of matter in the Universe on scales ranging from individual galaxies to superclusters and beyond.

This is important because, thanks to countless observations, we know that most of the matter in the Universe is “dark” and “cold”, meaning that it doesn’t emit light and moves very slowly.

We don’t yet understand what dark matter really is. Gravitational lensing is one way to try and find out more about it. Lensed images of galaxies can themselves be lensed, leading to distortions in the images known as shear and flexion. I’m trying to find out if these small, subtle effects can be seen and measured, and if so, what they might tell us about the nature of dark matter.

My career in brief

You can find all my published papers here and you can read and download my CV here.

You can find out more about what I am currently thinking and learning about on my blog. Below are some of my favourite posts.

All posts