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Radio Pulsar Populations

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arxiv 1903.06526 v2 pith:V5BGXOSJ submitted 2019-03-13 astro-ph.HE astro-ph.IMastro-ph.SR

Radio Pulsar Populations

classification astro-ph.HE astro-ph.IMastro-ph.SR
keywords populationradioneutronpopulationspulsarunderstandingableahead
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Our understanding of the neutron star population is informed to a great degree by large-scale surveys that have been carried out by radio facilities during the past fifty years. We summarize some of the recent breakthroughs in our understanding of the radio pulsar population and look ahead to future yields from upcoming experiments planned for the next decade. By the end of the 2020s, we anticipate a much more complete census of the Galactic population and being able to probe the populations of radio-emitting neutron stars more effectively in external galaxies. Among the anticipated discoveries are pulsar--black hole binary systems that will provide further tests of strong-field gravity, as well as large numbers of millisecond pulsars that are crucial to enhancing the sensitivity of timing arrays for low-frequency gravitational waves.

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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. Discovery and Timing of 49 Pulsars from the Arecibo 327-MHz Drift Survey

    astro-ph.HE 2025-02 accept novelty 5.0

    Reports timing solutions and basic properties for 49 pulsars (18 new) from the AO327 survey, with emission feature notes and model comparisons for distances.