Timing results of 22 years for PSR J0922+0638
arXiv:2506.22765 · doi:10.3847/1538-4357/adeb78
Abstract
We conducted a timing analysis of PSR J0922+0638 (B0919+06) using data from the Nanshan 26 m radio telescope and the MeerKAT telescope, spanning from January 2001 to March 2023. During this 22-year period, we discovered a previously unreported small glitch (glitch 1) before the well-known large glitch (glitch 2), occurring at , with a frequency jump amplitude of . We also identified ten slow glitch events, half of which were newly detected. These slow glitches occurred quasi-periodically, with an average interval of approximately 553(21) days, fractional frequency changes ranging from to , and a maximum fractional change in the first derivative of the frequency of . Additionally, our timing noise analysis reveals a change in the spectral index for noise power before and after glitch 2, with values of and , respectively, likely due to this large glitch. Throughout the entire observation period, the first derivative of the spin frequency () showed a periodic structure. The possible modulation period was estimated to be 537(24) days before the 700-day data gap at MJD 56716 and 600(58) days afterward. We discuss the periodic oscillations in pulsar rotation as a possible manifestation of spin-down noise and quasi-periodic slow glitches.
arXiv comment14 pages, 8 figures, 4 tables, ApJ (2025) accepted
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