Metallicity Constraints

Metallicity Constraints is a scientific construct in exoplanetary science that specifies the permissible range or bounds on the abundance of elements heavier than helium in an exoplanet’s atmosphere or host star, as inferred from infrared observational data, to inform planetary formation models and atmospheric characterization.

1.1K

Publications

86K

Citations

3.8K

Authors

891

Institutions

Publications per year

2017–2026

300

Authors

3.8K

  1. JJ
    Jonathan J. Fortney

    University of California, Santa Cruz, United States

    17 publications · 2.6K citations

    17

    h-index

  2. NC
    N. C. Santos

    Universidade do Porto, Portugal

    16 publications · 1.5K citations

    15

    h-index

  3. MM
    M. Mayor

    University of Geneva, Switzerland

    14 publications · 1.2K citations

    14

    h-index

  4. DQ
    D. Queloz

    University of Geneva, Switzerland

    14 publications · 1.2K citations

    14

    h-index

  5. FB
    F. Bouchy

    University of Geneva, Switzerland

    14 publications · 1.2K citations

    14

    h-index

1–5 of 3.8K

Venues

  1. The Astrophysical Journal

    ApJ · 343 publications · 33.6K citations

    101

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    206 publications · 14.5K citations

    66

    h-index

  3. Astronomy and Astrophysics

    188 publications · 13.8K citations

    65

    h-index

  4. The Astronomical Journal

    AJ · 83 publications · 5.6K citations

    38

    h-index

  5. The Astrophysical Journal Letters

    41 publications · 3.4K citations

    32

    h-index

1–5