Pulsar Timing Analysis

Pulsar Timing Analysis is a specialized methodology in gamma-ray data analysis that precisely measures the arrival times of pulsed electromagnetic radiation from rotating neutron stars to detect deviations induced by astrophysical phenomena, orbital dynamics, or gravitational waves, thereby enabling high-precision tests of fundamental physics and neutron star astrophysics.

849

Publications

57.7K

Citations

2.1K

Authors

672

Institutions

Publications per year

2017–2026

245

Authors

2.1K

  1. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    83 publications · 11.5K citations

    48

    h-index

  2. MK
    M. Krämer

    University of Manchester, United Kingdom

    67 publications · 8.6K citations

    42

    h-index

  3. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    49 publications · 5.7K citations

    36

    h-index

  4. VM
    V. M. Kaspi

    McGill University, Canada

    44 publications · 5.4K citations

    35

    h-index

  5. IH
    I. H. Stairs

    University of British Columbia, Canada

    49 publications · 7.9K citations

    34

    h-index

1–5 of 2.1K

Venues

  1. The Astrophysical Journal

    ApJ · 252 publications · 18.7K citations

    73

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    181 publications · 14.4K citations

    61

    h-index

  3. Astronomy and Astrophysics

    49 publications · 1.8K citations

    26

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 30 publications · 1.5K citations

    21

    h-index

  5. The Astrophysical Journal Letters

    27 publications · 2.8K citations

    20

    h-index

1–5