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| Main Authors: | , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2026
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2605.15724 |
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| _version_ | 1866910223588917248 |
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| author | Chen, Yujie Lian, Yujie Wang, Yujie Zhang, Liyun Qian, Lei Pan, Zhichen Cao, Shuo Yin, Dejiang Li, Baoda He, Ruili Liu, Tong Li, Wenze Zhang, Yichi Li, Yifeng Hao, Qiaoli Song, Jinyou Chen, Shuangyuan Wang, Xingyi Niu, Xianghua Guo, Minglei Huang, Menglin |
| author_facet | Chen, Yujie Lian, Yujie Wang, Yujie Zhang, Liyun Qian, Lei Pan, Zhichen Cao, Shuo Yin, Dejiang Li, Baoda He, Ruili Liu, Tong Li, Wenze Zhang, Yichi Li, Yifeng Hao, Qiaoli Song, Jinyou Chen, Shuangyuan Wang, Xingyi Niu, Xianghua Guo, Minglei Huang, Menglin |
| contents | Mildly recycled pulsars are neutron stars partially spun up through relatively short mass-transfer phases, typically with massive carbon-oxygen (CO) or oxygen-neon-magnesium (ONeMg) white dwarf companions. PSR J2338+4818, a mildly recycled pulsar, was discovered with the Five-hundred-meter Aperture Spherical Telescope (FAST). As a pilot study on the formation and evolutionary pathways of mildly recycled pulsars, we present the updated timing solution for PSR J2338+4818 and examine its single pulses and scintillation properties. Aided by the sensitivity of FAST, the single pulses of PSR J2338+4818 were systematically studied. 27,228 single pulses with S/N > 7 have been detected in our observations. For the FAST ultra-wideband observation on MJD 61045, the receiver was still in the technical commissioning phase, and then only a preliminary single-pulse search was performed. Pulse nulling was examined using a Markov Chain Monte Carlo (MCMC) method, but no evidence for nulling was found. The possible long-term nulling reported by previous studies did not occur in any of our observations in either the 1.0 to 1.5 GHz band or the 300 to 600 MHz band. Interstellar scintillation is evident in our observations. The measured scintillation timescales and bandwidths range from 2.93 to 25.26 minutes and 1.68 to 27.41 MHz, respectively. In all observations, no clear scintillation arc was found in the secondary spectra of PSR J2338+4818. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_15724 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | A Pilot Study of Mildly Recycled Pulsars: A Case Study of PSR J2338+4818 Chen, Yujie Lian, Yujie Wang, Yujie Zhang, Liyun Qian, Lei Pan, Zhichen Cao, Shuo Yin, Dejiang Li, Baoda He, Ruili Liu, Tong Li, Wenze Zhang, Yichi Li, Yifeng Hao, Qiaoli Song, Jinyou Chen, Shuangyuan Wang, Xingyi Niu, Xianghua Guo, Minglei Huang, Menglin High Energy Astrophysical Phenomena Mildly recycled pulsars are neutron stars partially spun up through relatively short mass-transfer phases, typically with massive carbon-oxygen (CO) or oxygen-neon-magnesium (ONeMg) white dwarf companions. PSR J2338+4818, a mildly recycled pulsar, was discovered with the Five-hundred-meter Aperture Spherical Telescope (FAST). As a pilot study on the formation and evolutionary pathways of mildly recycled pulsars, we present the updated timing solution for PSR J2338+4818 and examine its single pulses and scintillation properties. Aided by the sensitivity of FAST, the single pulses of PSR J2338+4818 were systematically studied. 27,228 single pulses with S/N > 7 have been detected in our observations. For the FAST ultra-wideband observation on MJD 61045, the receiver was still in the technical commissioning phase, and then only a preliminary single-pulse search was performed. Pulse nulling was examined using a Markov Chain Monte Carlo (MCMC) method, but no evidence for nulling was found. The possible long-term nulling reported by previous studies did not occur in any of our observations in either the 1.0 to 1.5 GHz band or the 300 to 600 MHz band. Interstellar scintillation is evident in our observations. The measured scintillation timescales and bandwidths range from 2.93 to 25.26 minutes and 1.68 to 27.41 MHz, respectively. In all observations, no clear scintillation arc was found in the secondary spectra of PSR J2338+4818. |
| title | A Pilot Study of Mildly Recycled Pulsars: A Case Study of PSR J2338+4818 |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2605.15724 |