Pulsar Timing Tests

Pulsar Timing Tests is a methodological framework within experimental tests of relativity that employs precise measurements of the arrival times of radio pulses from rotating neutron stars to detect deviations in orbital dynamics and gravitational wave signatures, thereby testing general relativistic predictions in strong-field regimes.

71

Publications

6.2K

Citations

451

Authors

235

Institutions

Publications per year

2017–2026

39

Authors

451

  1. MK
    M. Krämer

    University of Manchester, United Kingdom

    11 publications · 1.8K citations

    11

    h-index

  2. NW
    Norbert Wex

    Max Planck Institute for Radio Astronomy, Germany

    6 publications · 303 citations

    6

    h-index

  3. GH
    G. Hobbs

    Commonwealth Scientific and Industrial Research Organisation, Australia

    5 publications · 1.4K citations

    5

    h-index

  4. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    5 publications · 1.3K citations

    5

    h-index

  5. LS
    Lijing Shao

    Peking University, China

    5 publications · 266 citations

    5

    h-index

1–5 of 451

Venues

  1. Physical review. D/Physical review. D.

    PRD · 8 publications · 487 citations

    8

    h-index

  2. The Astrophysical Journal

    ApJ · 8 publications · 686 citations

    8

    h-index

  3. 4

    h-index

  4. Astronomy and Astrophysics

    3 publications · 192 citations

    3

    h-index

  5. International Journal of Modern Physics D

    3 publications · 274 citations

    3

    h-index

1–5