Binary Pulsar Timing

Binary Pulsar Timing is a method in experimental gravitation that precisely measures the arrival times of gamma-ray or radio pulses from a neutron star in a binary system to test predictions of general relativity, particularly gravitational wave emission and relativistic orbital dynamics.

920

Publications

70.8K

Citations

2.7K

Authors

690

Institutions

Publications per year

2017–2026

311

Authors

2.7K

  1. MK
    M. Krämer

    University of Manchester, United Kingdom

    99 publications · 12.7K citations

    53

    h-index

  2. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    71 publications · 8.3K citations

    46

    h-index

  3. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    73 publications · 9.2K citations

    45

    h-index

  4. IH
    I. H. Stairs

    University of British Columbia, Canada

    68 publications · 12.4K citations

    44

    h-index

  5. SM
    S. M. Ransom

    National Radio Astronomy Observatory, United States

    64 publications · 9K citations

    43

    h-index

1–5 of 2.7K

Venues

  1. The Astrophysical Journal

    ApJ · 267 publications · 19.8K citations

    75

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    171 publications · 13.1K citations

    62

    h-index

  3. Astronomy and Astrophysics

    47 publications · 3.2K citations

    27

    h-index

  4. The Astrophysical Journal Letters

    33 publications · 6.7K citations

    26

    h-index

  5. Nature

    28 publications · 3.6K citations

    24

    h-index

1–5