Pulse Profile Evolution

Pulse Profile Evolution is a temporal phenomenon in high-energy astrophysics characterized by systematic changes in the shape, phase, or amplitude of pulsed emission from rotating compact objects over time, as observed in gamma-ray and X-ray timing data.

434

Publications

19.7K

Citations

1.8K

Authors

558

Institutions

Publications per year

2017–2026

98

Authors

1.8K

  1. MK
    M. Krämer

    University of Manchester, United Kingdom

    20 publications · 1.3K citations

    19

    h-index

  2. BW
    B. W. Stappers

    University of Manchester, United Kingdom

    15 publications · 847 citations

    15

    h-index

  3. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    15 publications · 939 citations

    15

    h-index

  4. SJ
    S. Johnston

    Commonwealth Scientific and Industrial Research Organisation, Australia

    12 publications · 767 citations

    12

    h-index

  5. JW
    J. Wilms

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    12 publications · 373 citations

    12

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 114 publications · 6.4K citations

    45

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    85 publications · 3.3K citations

    35

    h-index

  3. Astronomy and Astrophysics

    27 publications · 1.2K citations

    21

    h-index

  4. The Astrophysical Journal Letters

    14 publications · 760 citations

    14

    h-index

  5. Optics Express

    11 publications · 497 citations

    11

    h-index

1–5