Stellar Radius Estimation

Stellar Radius Estimation is a computational method in astrophysics that determines the physical size of a star hosting an exoplanet by combining observational data with stellar models to distinguish it from alternative stellar parameter derivation techniques.

423

Publications

37.3K

Citations

1.7K

Authors

536

Institutions

Publications per year

2017–2026

137

Authors

1.7K

  1. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    25 publications · 2.8K citations

    24

    h-index

  2. JN
    Joshua N. Winn

    Massachusetts Institute of Technology, United States

    21 publications · 2.5K citations

    21

    h-index

  3. GT
    Guillermo Torres

    Center for Astrophysics Harvard & Smithsonian, United States

    19 publications · 2.7K citations

    19

    h-index

  4. DH
    Daniel Huber

    Aarhus University, Denmark

    19 publications · 2K citations

    18

    h-index

  5. MJ
    Matthew J. Holman

    Center for Astrophysics Harvard & Smithsonian, United States

    15 publications · 2.2K citations

    15

    h-index

1–5 of 1.7K

Venues

  1. The Astrophysical Journal

    ApJ · 130 publications · 16.6K citations

    67

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    61 publications · 3.7K citations

    34

    h-index

  3. Astronomy and Astrophysics

    56 publications · 3.3K citations

    33

    h-index

  4. The Astronomical Journal

    AJ · 39 publications · 3.6K citations

    27

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 12 publications · 327 citations

    11

    h-index

1–5