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In this study, we report on a detailed single pulse analysis of the radioemission from a rotating radio transient (RRAT) J1918$-$0449 which is the firstRRAT discovered with the five hundred meter aperture spherical radio telescope(FAST). The sensitive observations were carried out on 30 April 2021 using theFAST with a central frequency of 1250 MHz and a short time resolution of 49.152$\mu$s, which forms a reliable basis to probe single pulse emission propertiesin detail. The source was successively observed for around 2 hours. A total of83 dispersed bursts with significance above 6$\sigma$ are detected over 1.8hours. The source's DM and rotational period are determined to be 116.1$\pm$0.4\pcm \ and 2479.21$\pm$0.03 ms, respectively. The share of registered pulsesfrom the total number of observed period is 3.12\%. No underlying emission isdetected in the averaged off pulse profile. For bursts with fluence larger than10 Jy ms, the pulse energy follows a power-law distribution with an index of$-3.1\pm0.4$, suggesting the existence of bright pulse emission. We find thatthe distribution of time between subsequent pulses is consistent with astationary Poisson process and find no evidence of clustering over the 1.8 hobservations, giving a mean burst rate of one burst every 66 s. Closeinspection of the detected bright pulses reveals that 21 pulses exhibitwell-defined quasi-periodicities. The subpulse drifting is present innon-successive rotations with periodicity of $2.51\pm0.06$ periods. Finally,possible physical mechanisms are discussed.

astrophysical journal/the astrophysical journal

The discovery of a rotating radio transient J1918$-$0449 with intriguing  emission properties with the five hundred meter aperture spherical radio  telescope