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The FAST Galactic Plane Pulsar Snapshot survey: VI. The discovery of 473 new pulsars

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arxiv 2411.15961 v3 pith:CZUJNWZ3 submitted 2024-11-24 astro-ph.HE

The FAST Galactic Plane Pulsar Snapshot survey: VI. The discovery of 473 new pulsars

classification astro-ph.HE
keywords pulsarsfastsurveygppsdiscovereddiscoverygalacticplane
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is the most sensitive telescope at the $L$-band (1.0-1.5 GHz) and has been used to carry out the FAST Galactic Plane Pulsar Snapshot (GPPS) survey in the last 5 yr. Up to now, the survey has covered one-fourth of the planned areas within $\pm10^{\circ}$ from the Galactic plane visible by FAST, and discovered 751 pulsars. After the first publication of the discovery of 201 pulsars and one rotating radio transient (RRAT) in 2021 and 76 RRATs in 2023, here we report the discovery of 473 new pulsars from the FAST GPPS survey, including 137 new millisecond pulsars and 30 new RRATs. We find 34 millisecond pulsars discovered by the GPPS survey which can be timed with a precision better than 3 $\mu$s by using FAST 15 minute observations and can be used for pulsar timing arrays. The GPPS survey has discovered eight pulsars with periods greater than 10 s including one with 29.77 s. The integrated profiles of pulsars and individual pulses of RRATs are presented. During the FAST GPPS survey, we also detected previously known pulsars and updated parameters for 52 pulsars. In addition, we discovered two fast radio bursts plus one probable case with high dispersion measures indicating their extragalactic origin.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era

    astro-ph.HE 2026-07 accept novelty 2.5

    SKA1 AA* and AA4 will roughly double-to-triple the known pulsar population and supply thousands of new RMs, enabling detailed 3D mapping of Galactic disk and halo magnetic fields.