Variable Star Monitoring

Variable Star Monitoring is a systematic observational methodology in time-domain astronomy that involves the repeated measurement of stellar brightness over time to detect and characterize photometric variations indicative of intrinsic or extrinsic astrophysical processes.

135

Publications

5.9K

Citations

766

Authors

281

Institutions

Publications per year

2017–2026

17

Authors

766

  1. WH
    W. Herbst

    Wesleyan University, United States

    7 publications · 576 citations

    7

    h-index

  2. RT
    R. Titz

    Technische Universität Berlin, Germany

    4 publications · 88 citations

    4

    h-index

  3. TW
    T. W. S. Holoien

    Carnegie Observatories, United States

    4 publications · 665 citations

    4

    h-index

  4. JR
    John R. Percy

    University of Toronto, Canada

    4 publications · 108 citations

    4

    h-index

  5. PK
    P. Kábath

    Thüringer Landessternwarte Tautenburg, Germany

    4 publications · 88 citations

    4

    h-index

1–5 of 766

Venues

  1. The Astrophysical Journal

    ApJ · 27 publications · 1.1K citations

    18

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.4K citations

    17

    h-index

  3. The Astronomical Journal

    AJ · 21 publications · 1K citations

    17

    h-index

  4. Astronomy and Astrophysics

    12 publications · 850 citations

    12

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 18 publications · 498 citations

    12

    h-index

1–5