Timing Residuals

Timing Residuals is the difference between observed and predicted arrival times of gamma-ray photons, derived from a timing model, that quantifies deviations in pulsar or transient source emission as a function of time.

129

Publications

9.1K

Citations

441

Authors

226

Institutions

Publications per year

2017–2026

39

Authors

441

  1. MB
    M. Bailes

    Swinburne University of Technology, Australia

    12 publications · 1.4K citations

    12

    h-index

  2. GH
    G. Hobbs

    Commonwealth Scientific and Industrial Research Organisation, Australia

    12 publications · 1.9K citations

    12

    h-index

  3. WV
    W. van Straten

    Swinburne University of Technology, Australia

    9 publications · 1.3K citations

    9

    h-index

  4. FJ
    Fredrick Jenet

    West Virginia University, United States

    9 publications · 1.8K citations

    9

    h-index

  5. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    9 publications · 1.4K citations

    9

    h-index

1–5 of 441

Venues

  1. Monthly Notices of the Royal Astronomical Society

    40 publications · 3.1K citations

    28

    h-index

  2. The Astrophysical Journal

    ApJ · 26 publications · 1.8K citations

    21

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 8 publications · 276 citations

    8

    h-index

  4. Astronomy and Astrophysics

    7 publications · 500 citations

    7

    h-index

  5. 4

    h-index

1–5