Postgraduate research project

Uncovering extremely luminous flares from supermassive black holes with the world's largest telescopes

Funding
Competition funded View fees and funding
Type of degree
Doctor of Philosophy
Entry requirements
2:1 honours degree View full entry requirements
Faculty graduate school
Faculty of Engineering and Physical Sciences
Closing date

About the project

What happens when a giant star falls into a black hole? This project revolves around the most extreme events in the Universe. It uses cutting-edge analysis and machine learning techniques on data from the Rubin Observatory, and works alongside world experts, to understand the most luminous cosmic puzzle of our time.

Modern all-sky surveys are uncovering unusual, extremely luminous, long-lived flares in the centres of distant galaxies. Too bright to result from a single star’s death, they are more likely powered by violent accretion of material onto a supermassive black hole. This project aims to reveal what that material is and how it arrives, key to understanding black hole growth. 

Around 20 of these ambiguous nuclear transients (ANTs) are known, including the most energetic cosmic event ever observed, discovered by the BOB体育登录网址_欧宝体育官网平台-APP|下载 group. One possibility is that a massive star is torn apart by tidal forces, though how such stars reach the black hole remains unclear. Alternatively, they might involve instabilities in existing accretion disks—but the timescales appear too short. Many events show mid-infrared “echoes,” suggesting they are enshrouded in warm dust, perhaps some of which is falling in. 

BOB体育登录网址_欧宝体育官网平台-APP|下载 plays a leading role in two major facilities central to this project. The Rubin Observatory’s Legacy Survey of Space and Time (LSST) will discover millions of new astrophysical transients—supernovae, tidal disruptions, and hundreds of ANTs. BOB体育登录网址_欧宝体育官网平台-APP|下载 is also a core member of the Time Domain Extragalactic Survey (TiDES), which will obtain spectra of every ANT LSST finds. 

In this project, you will compare theoretical models with LSST light curves and TiDES spectra to measure the energy, black hole mass, and chemical composition of ANTs. You will also have opportunities to use world-class facilities such as the Very Large Telescope and James Webb Space Telescope, working in an international team with extensive opportunities for collaboration and travel.

As well as receiving core scientific training, you will:

  • develop advanced skills in statistical modelling, Bayesian inference, and data visualisation
  • gain experience with machine learning and AI methods applied to large datasets
  • build expertise in high-performance computing, programming (Python), and version control
  • have opportunities to present results through scientific papers, conferences, and outreach activities
  • strengthen transferable skills in teamwork, project management, and communication