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• W4386081666 abstract "In our work, we analyse $5times10^{4}$ single pulses from the recycled pulsar PSR J2222$-$0137 in one of its scintillation maxima observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). PSR J2222$-$0137 is one of the nearest and best studies of binary pulsars and a unique laboratory for testing gravitational theories. We report single pulses' energy distribution and polarization from the pulsar's main-pulse region. The single pulse energy follows the log-normal distribution. We resolve a steep polarization swing, but at the current time resolution ($64,mu{rm s}$), we find no evidence for the orthogonal jump in the main-pulse region, as has been suspected. We find a potential sub-pulse drifting period of $P_{3} sim 3.5,P$. We analyse the jitter noise from different integrated numbers of pulses and find that its $sigma_{j}$ is $270pm{9},{rm ns}$ for 1-hr integration at 1.25 GHz. This result is useful for optimizing future timing campaigns with FAST or other radio telescopes." @default.
• W4386081666 created "2023-08-23" @default.
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• W4386081666 date "2023-08-21" @default.
• W4386081666 modified "2023-10-16" @default.
• W4386081666 title "Variability, polarimetry, and timing properties of single pulses from PSR J2222-0137 using FAST" @default.
• W4386081666 doi "https://doi.org/10.48550/arxiv.2308.10683" @default.
• W4386081666 hasPublicationYear "2023" @default.
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