Variable Star Surveys

Variable Star Surveys is a systematic observational framework in survey astronomy designed to detect, monitor, and characterize stars exhibiting photometric variability over time, distinguished by its dedicated methodology for identifying temporal changes in stellar brightness across large sky areas.

388

Publications

22.5K

Citations

2.5K

Authors

579

Institutions

Publications per year

2017–2026

62

Authors

2.5K

  1. MC
    M. Catelan

    Pontificia Universidad Católica de Chile, Chile

    14 publications · 1.1K citations

    12

    h-index

  2. GP
    G. Pojmański

    University of Warsaw, Poland

    11 publications · 1.2K citations

    11

    h-index

  3. JL
    J. L. Prieto

    The Ohio State University, United States

    9 publications · 1.7K citations

    9

    h-index

  4. LE
    L. Eyer

    University of Geneva, Switzerland

    8 publications · 308 citations

    8

    h-index

  5. DM
    D. Minniti

    Pontificia Universidad Católica de Chile, Chile

    8 publications · 138 citations

    8

    h-index

1–5 of 2.5K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    71 publications · 3.5K citations

    35

    h-index

  2. The Astronomical Journal

    AJ · 63 publications · 5.6K citations

    34

    h-index

  3. The Astrophysical Journal

    ApJ · 45 publications · 3.1K citations

    29

    h-index

  4. Astronomy and Astrophysics

    37 publications · 1.1K citations

    23

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 37 publications · 2.1K citations

    17

    h-index

1–5