ASD Colloquium
Tuesday · 03:30 PM - 05:00 PM
Kaustubh Rajwade (University of Oxford)
Over the past two decades, wide-field radio surveys conducted with SKAO precursor facilities such as ASKAP, MeerKAT, and LOFAR have transformed our understanding of fast radio transients — millisecond to minute-duration bursts produced by some of the most extreme objects in the Universe. Among these are radio neutron stars and white dwarfs: pulsars, magnetars, rotating radio transients, and recently discovered long-period radio emitters that challenge traditional models of coherent radio emission.
In this talk, I will review how SKA precursor instruments have enabled systematic exploration of this diverse population and revealed intriguing connections between previously distinct sub-classes of radio neutron stars. The emerging picture suggests a continuum of behaviours, from classical pulsars to highly magnetised neutron stars (magnetars), with long-period transients occupying a newly recognised parameter space. I will discuss how these discoveries inform our understanding of radio emission from compact objects.
I will also discuss the recently discovered phenomenon of fast radio bursts (FRBs), which have opened a new frontier in high-energy astrophysics. By localising FRBs to distant galaxies and measuring their dispersion through intergalactic plasma, SKA precursors have demonstrated their power as cosmological probes — offering a novel means of tracing baryonic matter and studying the large-scale structure of the Universe.
Together, these advances illustrate how next-generation radio surveys are reshaping our view of compact objects and transforming fast radio transients from rare curiosities into precision tools for astrophysics and cosmology.