Eclipsing Binary Photometry

Eclipsing Binary Photometry is a specialized method within stellar photometry that measures and analyzes the periodic variations in a star's brightness caused by one stellar component eclipsing another in a binary system, enabling the determination of orbital and physical parameters of the stars.

336

Publications

13.7K

Citations

1.3K

Authors

443

Institutions

Publications per year

2017–2026

53

Authors

1.3K

  1. JS
    J. Southworth

    Keele University, United Kingdom

    15 publications · 955 citations

    14

    h-index

  2. GT
    Guillermo Torres

    Center for Astrophysics Harvard & Smithsonian, United States

    14 publications · 1.8K citations

    13

    h-index

  3. AC
    A. Claret

    Instituto de Astrofísica de Andalucía, Spain

    12 publications · 324 citations

    12

    h-index

  4. CH
    Claud H. Sandberg Lacy

    University of Arkansas at Fayetteville, United States

    12 publications · 479 citations

    12

    h-index

  5. MK
    M. Konacki

    Nicolaus Copernicus Astronomical Center, Poland

    9 publications · 200 citations

    9

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 63 publications · 3.4K citations

    30

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    66 publications · 2.1K citations

    25

    h-index

  3. Astronomy and Astrophysics

    41 publications · 1.4K citations

    23

    h-index

  4. The Astronomical Journal

    AJ · 60 publications · 2.2K citations

    23

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 19 publications · 311 citations

    13

    h-index

1–5