Transit Depth Analysis

Transit Depth Analysis is a quantitative method in exoplanetary science that measures the fractional decrease in a star's observed flux during a planetary transit to infer the relative size of an exoplanet with respect to its host star.

208

Publications

15.4K

Citations

877

Authors

368

Institutions

Publications per year

2017–2026

85

Authors

877

  1. DQ
    D. Queloz

    University of Geneva, Switzerland

    11 publications · 1.2K citations

    11

    h-index

  2. HA
    Heather A. Knutson

    California Institute of Technology, United States

    11 publications · 815 citations

    10

    h-index

  3. SU
    S. Udry

    University of Geneva, Switzerland

    10 publications · 1.5K citations

    10

    h-index

  4. PJ
    P. J. Wheatley

    University of Warwick, United Kingdom

    9 publications · 746 citations

    9

    h-index

  5. MG
    M. Gillon

    University of Liège, Belgium

    9 publications · 1.1K citations

    9

    h-index

1–5 of 877

Venues

  1. The Astrophysical Journal

    ApJ · 49 publications · 5.7K citations

    38

    h-index

  2. Astronomy and Astrophysics

    37 publications · 2.8K citations

    26

    h-index

  3. The Astronomical Journal

    AJ · 29 publications · 1.3K citations

    24

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    25 publications · 1.6K citations

    21

    h-index

  5. The Astrophysical Journal Letters

    18 publications · 1.2K citations

    17

    h-index

1–5