About
Juno Chan is a Research Fellow at the Niels Bohr Institute, University of Copenhagen, specializing in Theoretical High Energy, Astroparticle and Gravitational Physics. Holding a permanent position since 2025, Chan contributes to advanced research in gravitational wave astronomy and neutron star dynamics.
- Role: PhD Fellow (converted to Research Fellow)
- Location: Blegdamsvej 17, Copenhagen Ø
- Contact: chun.lung.chan@nbi.ku.dk, +45 35 32 87 21
Chan's research focuses on gravitational wave detection, neutron star magnetohydrodynamics, and gravitational lensing in astrophysical contexts. Key contributions include:
- Developing gravitational wave detection algorithms in lensed systems
- Modeling magnetized rotating neutron stars with relativistic MHD simulations
- Curating the LensCAT catalog for known gravitational lenses
- Multi-messenger lensing studies through LIGO-Virgo-KAGRA collaborations
Publications and Research Trends
Chan's 15 most recent publications (2023-2025) demonstrate expertise in gravitational wave astronomy, neutron star physics, and computational astrophysics. The work involves:
- Waveform analysis for lensed events
- MHD simulations of compact objects
- Multi-messenger lensing frameworks
- Signal processing for detector networks
- Cosmological implications of lensing
Collaborations span international institutions in gravitational wave networks, with frequent contributions to Physical Review D and Monthly Notices of the Royal Astronomical Society. No formal awards or student mentorship details are publicly available.
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