Continuous Gravitational Waves

Continuous Gravitational Waves is a theoretical astrophysical signal class within gravitational wave astronomy characterized by a nearly persistent, quasimonochromatic waveform originating from long-lived, non-axisymmetric rotating neutron stars or similar compact objects.

516

Publications

29.2K

Citations

8.7K

Authors

703

Institutions

Publications per year

2017–2026

238

Authors

8.7K

  1. AV
    A. Vecchio

    University of Birmingham, United Kingdom

    41 publications · 4.4K citations

    35

    h-index

  2. CP
    C. Palomba

    Sapienza University of Rome, Italy

    42 publications · 2.8K citations

    33

    h-index

  3. MA
    M. A. Papa

    Max Planck Institute for Gravitational Physics, Germany

    52 publications · 2.7K citations

    31

    h-index

  4. AM
    A. Melatos

    The University of Melbourne, Australia

    44 publications · 2.6K citations

    31

    h-index

  5. PL
    P. Leaci

    Sapienza University of Rome, Italy

    39 publications · 2.5K citations

    31

    h-index

1–5 of 8.7K

Venues

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

    PRD · 96 publications · 4.4K citations

    39

    h-index

  2. 26

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    32 publications · 1.3K citations

    23

    h-index

  4. The Astrophysical Journal

    ApJ · 26 publications · 1.4K citations

    22

    h-index

  5. Classical and Quantum Gravity

    33 publications · 1.3K citations

    20

    h-index

1–5