Binary Star Light Curves

Binary Star Light Curves is a time-series photometric measurement that represents the changes in apparent brightness of a binary star system over time due to mutual eclipses, orbital motions, and irradiation effects intrinsic to the system’s geometry and stellar components.

916

Publications

40.7K

Citations

2.4K

Authors

705

Institutions

Publications per year

2017–2026

125

Authors

2.4K

  1. SQ
    S.‐B. Qian

    Chinese Academy of Sciences, China

    36 publications · 1.2K citations

    22

    h-index

  2. JW
    Jae Woo Lee

    Korea Astronomy and Space Science Institute, South Korea

    25 publications · 795 citations

    18

    h-index

  3. RE
    R. E. Wilson

    University of Florida, United States

    21 publications · 2.5K citations

    18

    h-index

  4. LZ
    Li-Ying Zhu

    Chinese Academy of Sciences, China

    21 publications · 869 citations

    17

    h-index

  5. JH
    J.-J. He

    Chinese Academy of Sciences, China

    22 publications · 913 citations

    17

    h-index

1–5 of 2.4K

Venues

  1. The Astrophysical Journal

    ApJ · 180 publications · 11.9K citations

    54

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    169 publications · 7.4K citations

    45

    h-index

  3. The Astronomical Journal

    AJ · 171 publications · 8K citations

    42

    h-index

  4. Astronomy and Astrophysics

    108 publications · 4.9K citations

    32

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 52 publications · 1.8K citations

    22

    h-index

1–5