High-contrast Imaging

High-Contrast Imaging is a specialized observational technique in astronomical instrumentation that enables the direct detection of exoplanets by suppressing the overwhelming glare of their host stars to reveal faint nearby companions.

1.3K

Publications

76.1K

Citations

6K

Authors

1.5K

Institutions

Publications per year

2017–2026

477

Authors

6K

  1. OG
    Olivier Guyon

    National Astronomical Observatory of Japan, Japan

    75 publications · 3.8K citations

    31

    h-index

  2. DM
    Dimitri Mawet

    California Institute of Technology, United States

    52 publications · 2.5K citations

    26

    h-index

  3. MJ
    M. Janson

    Max Planck Institute for Astronomy, Germany

    38 publications · 2K citations

    25

    h-index

  4. LP
    Laurent Pueyo

    Space Telescope Science Institute, United States

    39 publications · 3.1K citations

    25

    h-index

  5. ES
    Eugene Serabyn

    Jet Propulsion Laboratory, United States

    42 publications · 2.2K citations

    25

    h-index

1–5 of 6K

Venues

  1. The Astrophysical Journal

    ApJ · 71 publications · 5.1K citations

    44

    h-index

  2. Astronomy and Astrophysics

    101 publications · 4.9K citations

    43

    h-index

  3. 31

    h-index

  4. Optics Express

    40 publications · 2.7K citations

    24

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 32 publications · 2.7K citations

    23

    h-index

1–5