Radio Properties of Rotating Radio Transients: Single Pulse Spectral and Wait Time Analyses
arXiv:1809.06729 · doi:10.3847/1538-4357/aae2b2
Abstract
Rotating radio transients (RRATs) are a sub-class of pulsars characterized by sporadic emission and thus can generally only be studied by analysis of their single-pulses. Here we present a single-pulse analysis using 11 years of timing data at 1400~MHz of three RRATs, PSRs~J18191458, J13175759, and J19131330. We perform a spectral analysis on the single-pulses of these RRATs for the first time, finding their mean spectral indices to be , , and respectively, within the known range of pulsar spectral indices. We find no evidence for narrowband features as seen for FRB~121102. However, we find the spread of single-pulse spectral indices for these RRATs (ranging from to ) to be larger than has been seen in other pulsars, with the exception of the Crab pulsar. We also analyze the time between detected pulses, or wait-time, and find that the pulses are not random and cluster around wait-times of a few pulse periods as well as pulse periods for PSRs~J18191458 and J13175759. Additionally we find that there is no correlation between the wait-time and pulse flux density. Finally we find that the distribution of the pulse energy for PSRs~J13175759 and J19131330 are log-normal, while that of PSR~J18191458 is log-normal with possible evidence of an additional power-law component.
arXiv comment16 pages, 11 figures, published in ApJ
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