Professor Bill Chaplin

Bill's research interests are focused on the study of the Sun and other Sun-like stars, with a particular interest in using asteroseismology to characterize newly discovered exoplanet systems with Sun-like hosts. He has leadership positions in Kepler/K2, TESS and PLATO, and is the principal-investigator on the BiSON project.

Dr Guy R. Davies

Guy is a lecturer at the University of Birmingham and he is interested in researching the nature of the Sun, stars that are a little bit like the Sun, and stars that are much more evolved than the Sun. He is interested in the evolution of stars and how the rotation, magnetism, and mass loss of stars evolves with time.  Guy uses observations of the oscillations of the Sun and the stars to learn about stellar evolution and to characterise the fundamental properties of stars.  The use of oscillations can be particularly valuable when studying stars that host extrasolar planets.  Guy is also involved with the daily operations of the BiSON project.

Professor Yvonne Elsworth FRS

Yvonne has previously been the head of the group and is now part-time and fully engaged with research. There are two primary strands to her research. The first is in helioseismology - the study of the interior of the Sun through the sound waves that propagate there. Associated with this is a strong interest in the instrumentation that enables the observations i.e., BiSON. The second strand is measurement of asteroseismic parameters and their use in the determination of the internal structure of red giants stars as key tracers of the structure of the galaxy. Yvonne is a Fellow of the Royal Society and currently vice-president of the Royal Astronomical Society.

In January 2020 Yvonne received the RAS Gold Medal. This is the highest award in the Society's gift, awarded for her achievements in helioseismology.

Professor Amaury Triaud - Head of Group

A regular visitor to observatories in the Atacama desert, Amaury is the discoverer of over one hundred exoplanets. His observations focus on planetary systems that are different compared to our own, either by the type of planets that compose those systems, by their architectures, or because of the type of star(s) they orbit. As part of the SPECULOOS collaboration, he now searches for planets the same size and the same temperature as the Earth and aims to find out if life emerged elsewhere in the Universe. The first such examples were found in the TRAPPIST-1 system.

In January 2020 Amaury received the Fowler award from the Royal Astronomical Society, and was named a finalist in the Blavatnik awards. Both recognise the important work done by young researchers across all of the physical sciences and engineering.

Postdoctoral researchers

Dr Warrick Ball

Warrick is a Research Fellow, and he is broadly interested in stellar modelling as a physical, numerical and mathematical problem. He has experience with computing models and their oscillations with several different codes. He uses asteroseismology of solar-like oscillators to improve stellar models, focusing most recently on models of near-surface convection in Sun-like stars.

Dr Rachel Howe

Rachel's main interests are the changes in the properties of solar oscillation modes in response to solar activity and the changes in the Sun's interior rotation over the solar cycle - in particular the pattern of migrating faster and slower flows known as the torsional oscillation. She is also interested in helioseismology using different observables such as the UV observations from SDO/AIA.

Dr Tanda Li

Tanda is currently a research fellow in the School and is focusing on theoretical modelling of solar-like oscillations. Tanda received his PhD degree in Beijing Normal University in 2008, and worked for National Astronomical Observatory in Beijing and University of Sydney afterwards. Tanda moved to Birmingham and joined the Solar & Stellar group in September 2019. Tanda's major interest is using asteroseismic modelling to provide accurate global parameters and internal structures for stars presenting solar-like oscillations. Recent researches include seismic mode identification and the modelling of Kepler subgiants and red giants, the ages of subgiants in Kepler and TESS field, and establishing theoretical model database for solar-like oscillators. 

Dr Martin Nielsen

Martin works on preparations for the ESA PLATO Mission, in particular the design, development and testing of "peak bagging" algorithms for extracting estimates of individual oscillation frequencies from PLATO data. This work involves use of machine-learning algorithms and hierarchical Bayesian models. Martin also works on analysing data from NASA's TESS spacecraft, and studying the rotation of stars similar to the Sun.

Dr Lalitha Sairam

Lalitha has worked extensively on both ground-based and space-based observations to understand the underlying physics of stellar atmospheres and their effects on orbiting exoplanets. Her focus areas include understanding stellar magnetic activity at the bottom of the main sequence. She also works on employing the computationally tractable probabilistic data analysis methods such as Gaussian processes to mitigate the effects of stellar activity on the planetary radial velocity signal. As part of the Solar & Stellar Physics group, Lalitha will be developing an analytical method to accurately measure the radial velocity of the double-line binaries.

Technical Staff

Dr Steven J. Hale CSci

Steven leads the operation and development of the international Birmingham Solar Oscillations Network (BiSON), a global network of automated robotic solar telescopes funded by the Science and Technology Facilities Council.  His research interests are instrumentation and electronics, and high-resolution optical spectroscopy techniques.

PhD Students

Lindsey Carboneau

Lindsey’s research is based on using asteroseismology as a window into the evolution of stars. With the combination of asteroseismology on large, high-quality data sets and computationally advanced statistical techniques, we will gain a better understanding of stellar properties and therefore the structure and evolution of the galaxy.  She is also working with the TESS Asteroseismic Science Operations Center to develop a photometry pipeline tailored towards providing high-precision data for asteroseismology on stars from the NASA TESS mission.

Georgina Dransfield

Georgina is predominantly interested in exoplanets and how we can group them together. Classification of objects like stars, planets and moons allow us to make predictions about how they were formed and what they are made of. Georgina is looking at where exoplanets fit in with populations of well-studied objects in order to learn more about the atmospheres of exoplanets. This is particularly interesting, as better techniques to determine whether or not a planet has, for example, water in its atmosphere will allow us to spot potential candidates for sustaining life.

Alexander Lyttle

Alex is using machine learning with stellar models to speed up the inference of fundamental stellar parameters. Using asteroseismology from NASA’s Kepler and TESS missions with astrometry from ESA’s Gaia mission, he hopes to develop robust statistical methods to determine how helium abundance varies in the Milky Way. His other research interests include probing the physics of stellar interiors using asteroseismology and contributing to open source software in astronomy. One such software is the python package PBjam which, for example, he uses to measure the oscillation modes of exoplanet host stars and subgiants.

Matthew Standing

Matthew’s research interests focus on exoplanet discovery using the radial velocity method, specifically around binary star systems. Only a few of these “circumbinary” planets have been discovered so far, however many more are predicted to exist. Finding these predicted planets could help shed some light on how planetary systems form and evolve over time. To find these planets Matt gathers data from telescopes such as the High Accuracy Radial velocity Planet Searcher (HARPS) located at the La Silla Observatory in Chile.

Walter Van Rossem

Walter's primary research interest lies in stellar modelling and asteroseismology. Combining these two he is looking for asteroseismic signatures for stellar mergers using MESA and GYRE for stars a bit more massive than the Sun.

Emma Willett

Emma Started working in the group during her Master’s project, during which she investigated the helium abundance in red clump stars. She is now working on asterochronometry – a project to measure the ages of stars more precisely and accurately using data from asteroseismology and other sources. These ages are important for many fields within astrophysics. For example, we can use them for galactic archaeology to understand the formation and evolution of the Milky Way and to study systems of planets around other stars.

Artist in Collaboration

Caroline Devine

Administrative Staff

Mrs Louise Barden (Secretary to the Group)