An analysis of the time-frequency structure of several bursts from FRB121102 detected with MeerKAT
arXiv:2105.11822 · doi:10.1093/mnras/stab1544
Abstract
We present a detailed study of the complex time-frequency structure of a sample of previously reported bursts of FRB 121102 detected with the MeerKAT telescope in September 2019. The wide contiguous bandwidth of these observations have revealed a complex bifurcating structure in some bursts at MHz. When de-dispersed to their structure-optimised dispersion measures, two of the bursts show a clear deviation from the cold plasma dispersion relationship below MHz. We find a differential dispersion measure of pc cm between the lower and higher frequency regions of each burst. We investigate the possibility of plasma lensing by Gaussian lenses of AU in the host galaxy, and demonstrate that they can qualitatively produce some of the observed burst morphologies. Other possible causes for the observed frequency dependence, such as Faraday delay, are also discussed. Unresolved sub-components in the bursts, however, may have led to an incorrect DM determination. We hence advise exercising caution when considering bursts in isolation. We analyse the presence of two apparent burst pairs. One of these pairs is a potential example of upward frequency drift. The possibility that burst pairs are echoes is also discussed. The average structure-optimised dispersion measure is found to be pc cm consistent with the values reported in 2018. We use two independent methods to determine the structure-optimised dispersion measure of the bursts: the DM_phase algorithm and autocorrelation functions. The latter originally developed for pulsar analysis is applied to FRBs for the first time in this paper.
arXiv comment13 pages, 12 figures. Accepted for publication in MNRAS
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