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Gravitational wave research using pulsar timing arrays

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arxiv 1707.01615 v2 pith:MLZIXKKC submitted 2017-07-06 astro-ph.IM astro-ph.HE

classification astro-ph.IMastro-ph.HE
keywords timingarraypulsargravitationalwavearrayscurrentdiscuss
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A pulsar timing array (PTA) refers to a program of regular, high-precision timing observations of a widely distributed array of millisecond pulsars. Here we review the status of the three primary PTA projects and the joint International Pulsar Timing Array project. We discuss current results related to ultra-low-frequency gravitational wave searches and highlight opportunities for the near future.

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Forward citations

Cited by 2 Pith papers

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

  1. First fast radio burst search campaign at the Argentine Institute of Radio Astronomy

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    The IAR campaign found one FRB candidate with DM 243 pc cm^-3 and S/N 8.2, backed by successful recovery of archival and injected bursts.

  2. Upgraded antennas for pulsar observations in the Argentine Institute of Radio astronomy

    astro-ph.IM 2019-08 conditional novelty 6.0 of 10

    IAR's upgraded 30 m antennas achieve sub-microsecond pulsar timing on J0437-4715 and detected the 2019 Vela glitch, establishing a new southern-hemisphere daily pulsar monitoring capability.

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