Adaptive Optics

Adaptive Optics is a branch of optical instrumentation within Observational Astronomy that employs real-time wavefront sensing and deformable mirrors to dynamically correct atmospheric distortions in astronomical observations, thereby enhancing the spatial resolution of ground-based telescopes in both optical and infrared wavelengths.

5.3K

Publications

227.7K

Citations

14.3K

Authors

2.2K

Institutions

Publications per year

2017–2026

1.3K

Authors

14.3K

  1. MJ
    Martin J. Booth

    University of Oxford, United Kingdom

    58 publications · 5.4K citations

    37

    h-index

  2. BL
    Brent L. Ellerbroek

    TMT Observatory, United States

    91 publications · 3.4K citations

    34

    h-index

  3. TF
    Thierry Fusco

    Office National d'Études et de Recherches Aérospatiales, France

    121 publications · 4.9K citations

    34

    h-index

  4. NH
    N. Hubin

    European Southern Observatory, Germany

    94 publications · 3.3K citations

    31

    h-index

  5. OG
    Olivier Guyon

    National Astronomical Observatory of Japan, Japan

    77 publications · 3.3K citations

    30

    h-index

1–5 of 14.3K

Venues

  1. Optics Express

    467 publications · 25K citations

    80

    h-index

  2. The Astrophysical Journal

    ApJ · 153 publications · 10.4K citations

    66

    h-index

  3. Journal of the Optical Society of America A

    223 publications · 14.1K citations

    63

    h-index

  4. 62

    h-index

  5. Optics Letters

    255 publications · 12.2K citations

    60

    h-index

1–5