Active Galactic Nuclei Variability

Active Galactic Nuclei Variability is a time-domain astronomical phenomenon characterized by fluctuations in the electromagnetic emission of active galactic nuclei due to changes in accretion dynamics, relativistic jet activity, or obscuration processes near the central supermassive black hole.

1.5K

Publications

115.7K

Citations

5.7K

Authors

1K

Institutions

Publications per year

2017–2026

435

Authors

5.7K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    35 publications · 3.1K citations

    31

    h-index

  2. BM
    B. M. Peterson

    The Ohio State University, United States

    34 publications · 7.5K citations

    31

    h-index

  3. KH
    K. Horne

    University of St Andrews, United Kingdom

    21 publications · 2K citations

    19

    h-index

  4. WK
    W. Kollatschny

    University of Göttingen, Germany

    21 publications · 2K citations

    19

    h-index

  5. AC
    A. Comastri

    Osservatorio astronomico di Bologna, Italy

    18 publications · 1.9K citations

    18

    h-index

1–5 of 5.7K

Venues

  1. The Astrophysical Journal

    ApJ · 508 publications · 42.4K citations

    108

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    361 publications · 23.9K citations

    78

    h-index

  3. Astronomy and Astrophysics

    168 publications · 9.5K citations

    52

    h-index

  4. The Astrophysical Journal Supplement Series

    53 publications · 5.9K citations

    37

    h-index

  5. The Astronomical Journal

    AJ · 44 publications · 4.5K citations

    28

    h-index

1–5