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FAST pulsar database: I. Polarization profiles of 682 pulsars

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arxiv 2307.10340 v1 pith:6XBPPNSE submitted 2023-07-14 astro-ph.HE hep-exhep-ph

FAST pulsar database: I. Polarization profiles of 682 pulsars

P. F. Wang , J. L. Han , J. Xu , C. Wang , Y. Yan , W. C. Jing , W. Q. Su , D. J. Zhou
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T. Wang
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classification astro-ph.HE hep-exhep-ph
keywords polarizationprofilespulsarssomepulsarcomponentsfastangle
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Pulsar polarization profiles are very basic database for understanding the emission processes in pulsar magnetosphere. After careful polarization calibration of the 19-beam L-band receiver and verification of beam-offset observation results, we obtain polarization profiles of 682 pulsars from observations by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) during the survey tests for the Galactic Plan Pulsar Snapshot (GPPS) survey and other normal FAST projects. Among them, polarization profiles of about 460 pulsars are observed for the first time. The profiles exhibit diverse features. Some pulsars have a polarization position angle curve with a good S-shaped swing, and some with orthogonal modes; some have components with highly linearly components or strong circularly polarized components; some have a very wide profile, coming from an aligned rotator, and some have an interpulse from a perpendicular rotator; some wide profiles are caused by interstellar scattering. We derive geometry parameters for 190 pulsars from the S-shaped position angle curves or with orthogonal modes. We find that the linear and circular polarization or the widths of pulse profiles have various frequency dependencies. Pulsars with large fraction of linear polarization are more likely to have a large Edot.

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Cited by 4 Pith papers

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    astro-ph.HE 2026-07 conditional novelty 6.0

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