Searching for the spectral depolarisation of ASKAP one-off FRB sources
Pavan A. Uttarkar, R. M. Shannon, K. Gourdji, A. T. Deller, C. K. Day,, S. Bhandari

TL;DR
This study investigates the spectral depolarisation of five one-off FRBs and one repeating FRB using ASKAP data, finding no evidence of depolarisation and suggesting environmental differences between one-off and repeating FRBs.
Contribution
First spectro-polarimetric analysis of a small sample of one-off FRBs, providing constraints on their depolarisation properties and environmental characteristics.
Findings
No spectral depolarisation detected in the sample.
Constraints on $\sigma_{ m RM}$ are much smaller than those of repeating FRBs.
Results support environmental differences between one-off and repeating FRBs.
Abstract
Fast Radio Bursts (FRBs) are extragalactic transients of (sub-)millisecond duration that show wide-ranging spectral, temporal, and polarimetric properties. The polarimetric analysis of FRBs can be used to probe intervening media, study the emission mechanism, and test possible progenitor models. In particular, low frequency depolarisation of FRBs can identify dense, turbulent, magnetised, ionised plasma thought to be near the FRB progenitor. An ensemble of repeating FRBs has shown low-frequency depolarisation. The depolarisation is quantified by the parameter , which correlates with proxies for both the turbulence and mean magnetic field strength of the putative plasma. However, while many non-repeating FRBs show comparable scattering (and hence inferred turbulence) to repeating FRBs, it is unclear whether their surrounding environments are comparable to those of…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · GNSS positioning and interference · Radio Astronomy Observations and Technology
