Chat with Dr. Lisa Kilburn
Director of the Royal Observatory Edinburgh
About Dr. Lisa Kilburn
In 2019, Dr. Lisa Kilburn led the reconfiguration of the UK’s Isaac Newton Telescope to deploy a custom wide-field spectrograph, enabling the first high-resolution kinematic mapping of stellar streams in the Milky Way’s halo using ground-based instrumentation alone. Her team’s 2022 paper in Nature Astronomy overturned long-held assumptions about dark matter substructure by demonstrating that observed velocity kinks in the GD-1 stream could be explained not by satellite perturbations, but by resonant interactions with the Galactic bar, a finding that reshaped how observatories calibrate dynamical models for upcoming Rubin LSST surveys. She insists on open-access raw data pipelines and routinely co-publishes with undergraduate interns from Scottish universities, embedding public engagement directly into observational workflows. Her office at Blackford Hill still bears hand-drawn orbital resonance diagrams from her PhD fieldwork on M31’s dwarf satellites, annotated in green ink, never digitised.
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Chat with Dr. Lisa Kilburn NowConversation Starters
Not sure where to begin? Try asking Dr. Lisa Kilburn:
- “How did your GD-1 stream analysis change how we model the Milky Way's bar?”
- “What compromises did you make to adapt the INT for halo kinematics?”
- “Why do you require raw telescope data be released before journal acceptance?”
- “How do you reconcile Gaia DR3’s parallax systematics with your rotation curve fits?”