Ultra-Wideband Polarimetry of the April 2021 Profile Change Event in PSR J1713+0747
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866914253314719744 |
|---|---|
| author | Mandow, Rami F. Zic, Andrew Dawson, J. R. Wang, Shuangqiang Curylo, Malgorzata Dai, Shi Di Marco, Valentina Hobbs, George Gupta, Vivek Kapur, Agastya Kerr, M. Lower, Marcus E. Mishra, Saurav Reardon, Daniel Russell, Christopher J. Shannon, Ryan M. Zhang, Lei Zhu, Xingjiang |
| author_facet | Mandow, Rami F. Zic, Andrew Dawson, J. R. Wang, Shuangqiang Curylo, Malgorzata Dai, Shi Di Marco, Valentina Hobbs, George Gupta, Vivek Kapur, Agastya Kerr, M. Lower, Marcus E. Mishra, Saurav Reardon, Daniel Russell, Christopher J. Shannon, Ryan M. Zhang, Lei Zhu, Xingjiang |
| contents | The millisecond pulsar PSR J1713+0747 is a high-priority target for pulsar timing array experiments due to its long-term timing stability, and bright, narrow pulse profile. In April 2021, PSR~J1713$+$0747 underwent a significant profile change event, observed by several telescopes worldwide. Using the broad-bandwidth and polarimetric fidelity of the Ultra-Wideband Low-frequency receiver on Murriyang, CSIRO's Parkes radio telescope, we investigated the long-term spectro-polarimetric behaviour of this profile change in detail. We highlight the broad-bandwidth nature of the event, which exhibits frequency dependence that is inconsistent with cold-plasma propagation effects. We also find that spectral and temporal variations are stronger in one of the orthogonal polarisation modes than the other, and observe mild variations ($\sim 3$ - $5\,σ$ significance) in circular polarisation above 1400 MHz following the event. However, the linear polarisation position angle remained remarkably stable in the profile leading edge throughout the event. With over three years of data post-event, we find that the profile has not yet recovered back to its original state, indicating a long-term asymptotic recovery, or a potential reconfiguration of the pulsar's magnetic field. These findings favour a magnetospheric origin of the profile change event over a line-of-sight propagation effect in the interstellar medium. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_18972 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Ultra-Wideband Polarimetry of the April 2021 Profile Change Event in PSR J1713+0747 Mandow, Rami F. Zic, Andrew Dawson, J. R. Wang, Shuangqiang Curylo, Malgorzata Dai, Shi Di Marco, Valentina Hobbs, George Gupta, Vivek Kapur, Agastya Kerr, M. Lower, Marcus E. Mishra, Saurav Reardon, Daniel Russell, Christopher J. Shannon, Ryan M. Zhang, Lei Zhu, Xingjiang High Energy Astrophysical Phenomena Solar and Stellar Astrophysics The millisecond pulsar PSR J1713+0747 is a high-priority target for pulsar timing array experiments due to its long-term timing stability, and bright, narrow pulse profile. In April 2021, PSR~J1713$+$0747 underwent a significant profile change event, observed by several telescopes worldwide. Using the broad-bandwidth and polarimetric fidelity of the Ultra-Wideband Low-frequency receiver on Murriyang, CSIRO's Parkes radio telescope, we investigated the long-term spectro-polarimetric behaviour of this profile change in detail. We highlight the broad-bandwidth nature of the event, which exhibits frequency dependence that is inconsistent with cold-plasma propagation effects. We also find that spectral and temporal variations are stronger in one of the orthogonal polarisation modes than the other, and observe mild variations ($\sim 3$ - $5\,σ$ significance) in circular polarisation above 1400 MHz following the event. However, the linear polarisation position angle remained remarkably stable in the profile leading edge throughout the event. With over three years of data post-event, we find that the profile has not yet recovered back to its original state, indicating a long-term asymptotic recovery, or a potential reconfiguration of the pulsar's magnetic field. These findings favour a magnetospheric origin of the profile change event over a line-of-sight propagation effect in the interstellar medium. |
| title | Ultra-Wideband Polarimetry of the April 2021 Profile Change Event in PSR J1713+0747 |
| topic | High Energy Astrophysical Phenomena Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2509.18972 |