Discovery of Two Highly Scattered Pulsars from Image-Based Circular Polarization Searches with the Australian SKA Pathfinder
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| Main Authors: | , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866911516723249152 |
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| author | Sengar, Rahul Kaplan, David L. Lenc, Emil Anumarlapudi, Akash Hurley-Walker, Natasha Wang, Ziteng Driessen, Laura Dobie, Dougal Murphy, Tara |
| author_facet | Sengar, Rahul Kaplan, David L. Lenc, Emil Anumarlapudi, Akash Hurley-Walker, Natasha Wang, Ziteng Driessen, Laura Dobie, Dougal Murphy, Tara |
| contents | We report the discovery and timing of two pulsars from a sample of four circularly polarized sources identified in radio continuum images taken as part of the Australian SKA Pathfinder (ASKAP) Variables and Slow Transients (VAST) survey. Observations with the Parkes (Murriyang) radio telescope confirmed both sources as normal pulsars with high dispersion measures. PSR J1646$-$4451 has a spin period of 217 ms and a dispersion measure (DM) of 928 $\rm cm^{-3} \, pc$, while PSR J1837$-$0616 exhibits a spin period of 118 ms and a DM of 793 $\rm cm^{-3} pc$. These pulsars show extreme pulse broadening due to scattering, with measured scattering timescales of 117 ms and 75 ms at observing frequencies of $\sim$ 1.8 GHz, respectively. These measurements imply extrapolated scattering timescales at 1 GHz of $\sim$1346 ms and 740 ms, placing them among the most heavily scattered known pulsars. Our findings underscore the potential of using circular polarization in radio continuum images as a tool for identifying highly scattered pulsars. Future wide-field radio continuum surveys are poised to uncover a broader population of extreme pulsars, particularly those that are heavily scattered at 1.4 GHz, intrinsically faint, or residing in binaries$-$offering valuable insights into both pulsar demographics and the complex structure of the ionized interstellar medium. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2509_20611 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Discovery of Two Highly Scattered Pulsars from Image-Based Circular Polarization Searches with the Australian SKA Pathfinder Sengar, Rahul Kaplan, David L. Lenc, Emil Anumarlapudi, Akash Hurley-Walker, Natasha Wang, Ziteng Driessen, Laura Dobie, Dougal Murphy, Tara High Energy Astrophysical Phenomena We report the discovery and timing of two pulsars from a sample of four circularly polarized sources identified in radio continuum images taken as part of the Australian SKA Pathfinder (ASKAP) Variables and Slow Transients (VAST) survey. Observations with the Parkes (Murriyang) radio telescope confirmed both sources as normal pulsars with high dispersion measures. PSR J1646$-$4451 has a spin period of 217 ms and a dispersion measure (DM) of 928 $\rm cm^{-3} \, pc$, while PSR J1837$-$0616 exhibits a spin period of 118 ms and a DM of 793 $\rm cm^{-3} pc$. These pulsars show extreme pulse broadening due to scattering, with measured scattering timescales of 117 ms and 75 ms at observing frequencies of $\sim$ 1.8 GHz, respectively. These measurements imply extrapolated scattering timescales at 1 GHz of $\sim$1346 ms and 740 ms, placing them among the most heavily scattered known pulsars. Our findings underscore the potential of using circular polarization in radio continuum images as a tool for identifying highly scattered pulsars. Future wide-field radio continuum surveys are poised to uncover a broader population of extreme pulsars, particularly those that are heavily scattered at 1.4 GHz, intrinsically faint, or residing in binaries$-$offering valuable insights into both pulsar demographics and the complex structure of the ionized interstellar medium. |
| title | Discovery of Two Highly Scattered Pulsars from Image-Based Circular Polarization Searches with the Australian SKA Pathfinder |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2509.20611 |