FRB 20230708A, a quasi-periodic FRB with unique temporal-polarimetric morphology
T. Dial, A. T. Deller, P. A. Uttarkar, M. E. Lower, R. M. Shannon,, Kelly Gourdji, Lachlan Marnoch, A. Bera, Stuart D. Ryder, Marcin Glowacki, J., Xavier Prochaska

TL;DR
This paper reports the detection of a quasi-periodic fast radio burst with unique temporal and polarimetric features, providing insights into its possible magnetar origin and the role of microstructure in emission morphology.
Contribution
It presents the first detailed temporal-polarimetric analysis of FRB 20230708A, including modeling of periodicity, scattering, scintillation, and polarization effects.
Findings
Potential 7.267 ms periodicity with low significance
High circular polarization not caused by Faraday conversion
Properties consistent with a magnetar model involving microstructure
Abstract
There has been a rapid increase in the known fast radio burst (FRB) population, yet the progenitor(s) of these events have remained an enigma. A small number of FRBs have displayed some level of quasi-periodicity in their burst profile, which can be used to constrain their plausible progenitors. However, these studies suffer from the lack of polarisation data which can greatly assist in constraining possible FRB progenitors and environments. Here we report on the detection and characterisation of FRB 20230708A by the Australian Square Kilometre Array Pathfinder (ASKAP), a burst which displays a rich temporal and polarimetric morphology. We model the burst time series to test for the presence of periodicity, scattering and scintillation. We find a potential period of T = 7.267 ms within the burst, but with a low statistical significance of 1.77. Additionally, we model the burst's…
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Taxonomy
TopicsAstro and Planetary Science
