Over the last several years, new instrumentation on interferometers such as the VLA and ASKAP has enabled (sub-)arcsecond localisations of Fast Radio Bursts (FRBs) upon discovery. This sample of well-localised FRBs is crucial for progenitor identifications and constraints, as it allows follow-up observations at other wavelengths. While no contemporaneous, transient multi-wavelength counterparts to FRBs have been identified yet, a couple of well-localised, prolific repeating FRBs have been associated with milliarcsecond-scale continuum radio sources ("persistent sources"). Magnetar-based models for FRB progenitors can account for co-located persistent radio emission, but generally expect a correlation between the persistent source properties and FRB source age, which itself is often assumed to correlate with repetition properties. We have recently identified persistent radio emission, sub-arcsecond in size, whose position is consistent with that of the (so-far) non-repeating FRB 20190714A. We propose to observe this persistent source with the HSA to confirm the association, and study the compactness and nature of this source. If confirmed as a milli-arcsecond scale persistent source associated with the FRB, this first detection from a non-repeating FRB will have profound implications for FRB progenitor models.
Name | Institution |
---|---|
Casey Law | California Institute of Technology |
Manisha Caleb * | Australian National University; Sydney, University of |
Adam Deller | Swinburne University of Technology |
Ben Stappers | Manchester, University of |
James Chibueze | Kagoshima University; Square Kilometre Array |
Ryan Shannon | Swinburne University of Technology |
Keith Bannister | Australia Telescope National Facility |
Rene Breton | Toronto, University of; Southampton, University of |
Elizabeth Mahony | Netherlands Institute for Radio Astronomy; Sydney, University of; Commonwealth Scientific and Industrial Research Organisation |
GBT Operator | Green Bank Observatory |
* indicates the PI