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Dr. Ashley Ruiter is a Senior Lecturer and Australian Research Council (ARC) Future Fellow in the School of Science at the University of New South Wales (UNSW) Canberra, where she also serves as Physics & Oceanography Stream Coordinator and contributes to the Astronomy & Astrophysics research group. She earned her BSc (Honours) in 2002 from York University in Toronto, Canada, MSc in 2005 from Saint Mary’s University in Halifax, Nova Scotia, Canada, and PhD in 2009 from New Mexico State University in the USA, completing the final year of her doctorate at the Harvard-Smithsonian Center for Astrophysics. Her postdoctoral positions include a fellowship from 2009 to 2014 in the supernova group at the Max Planck Institute for Astrophysics in Garching, Germany, and from 2014 to 2017 at the Research School of Astronomy and Astrophysics (Mount Stromlo) at the Australian National University, funded by CAASTRO. In 2017, she commenced her ARC Future Fellowship at UNSW Canberra, holding a concurrent visiting role at the Australian National University’s Mathematical Sciences Institute.
Ruiter’s research focuses on the astrophysics of interacting binary stars, employing binary population synthesis models to connect progenitors to supernovae and transients, including Type Ia supernovae, R Coronae Borealis stars, AM CVn binaries, novae, and accretion-induced collapse to neutron stars. She investigates occurrence rates, delay times, explosion locations, stellar properties, and nucleosynthesis, with applications to gravitational wave sources detectable by LISA. Key publications include “Type Ia supernova progenitors: a contemporary view of a long-standing puzzle” (Astronomy & Astrophysics Review, 2025, co-authored with I. R. Seitenzahl), “Rates and Delay Times of Type Ia Supernovae” (Astrophysical Journal, 2009, 390 citations), “Type Ia supernova sub-classes and progenitor origin” (Proceedings of the International Astronomical Union, 2019, 103 citations), and “Can Neutron Star Mergers Alone Explain the r-process Enrichment of the Milky Way?” (Astrophysical Journal Letters, 2023, 51 citations). Her body of work has amassed over 11,300 citations with an h-index of 49. Ruiter supervises three PhD students and one honours student, and co-led the Transients Down Under conference in 2024. She engages in public outreach via UNSW’s Ask an Expert series on topics such as stellar life cycles and gravitational waves.