Transit Depth Variations

Transit Depth Variations is a measurement metric in exoplanetary science that quantifies the differences in the apparent depth of an exoplanet's transit as observed at various wavelengths or observational epochs, enabling the detection of atmospheric opacity changes due to molecular absorption, scattering, or stellar photospheric inhomogeneities.

176

Publications

15K

Citations

771

Authors

332

Institutions

Publications per year

2017–2026

69

Variants

Transit Depth Variation

Authors

771

  1. JJ
    Jonathan J. Fortney

    University of California, Santa Cruz, United States

    10 publications · 765 citations

    10

    h-index

  2. HA
    Heather A. Knutson

    California Institute of Technology, United States

    11 publications · 792 citations

    10

    h-index

  3. PJ
    P. J. Wheatley

    University of Warwick, United Kingdom

    9 publications · 864 citations

    9

    h-index

  4. DK
    David K. Sing

    University of Exeter, United Kingdom

    8 publications · 1.2K citations

    8

    h-index

  5. IJ
    Ian J. M. Crossfield

    California Institute of Technology, United States

    8 publications · 641 citations

    8

    h-index

1–5 of 771

Venues

  1. The Astrophysical Journal

    ApJ · 43 publications · 5.4K citations

    37

    h-index

  2. Astronomy and Astrophysics

    29 publications · 2.8K citations

    23

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.5K citations

    23

    h-index

  4. The Astronomical Journal

    AJ · 25 publications · 1.2K citations

    22

    h-index

  5. The Astrophysical Journal Letters

    17 publications · 1.1K citations

    16

    h-index

1–5