Ziggy Pleunis is an assistant professor in high-energy astrophysics and an NWO Veni fellow at the University of Amsterdam and a visiting scientist at ASTRON, Netherlands Institute for Radio Astronomy. He obtained his PhD from McGill University in 2020 on the detection and characterization of fast radio bursts with the CHIME telescope. His thesis work was recognized with prizes from IAU Division D and the Canadian Astronomical Society. Ziggy was an independent Dunlap postdoctoral fellow at the University of Toronto's Dunlap Institute for Astronomy & Astrophysics in Canada until starting at UvA/ASTRON in January 2024.
Ziggy’s research focuses on the detection and characterization of fast radio bursts. It is his ambition to unravel the origins of these extragalactic transients and to develop their use as astrophysical tools to better understand the Universe at large. He is mainly a radio astronomer, but has a broad experience across wavelengths, having led and collaborated in studies on pulsars and fast radio bursts using data collected with the CHIME, LOFAR, Arecibo, Green Bank, Fermi and optical telescopes. He is a member of the CHIME/FRB Collaboration and has helped to design, build, and commission the CHIME/FRB experiment during his PhD at McGill University. He is also part of the team that has discovered the lowest-frequency millisecond pulsars and fast radio bursts with the LOFAR telescope.
Fast radio bursts, neutron stars, astrophysical transients, radio astronomy.