Microlensing Astrometry

Microlensing Astrometry is a space-based astrometric method that precisely measures the apparent positional shift of a background star caused by the gravitational deflection of light due to a foreground lensing object, enabling the detection and characterization of dark or faint astronomical bodies such as exoplanets and stellar remnants.

95

Publications

4.5K

Citations

415

Authors

199

Institutions

Publications per year

2017–2026

21

Authors

415

  1. AU
    A. Udalski

    University of Warsaw, Poland

    14 publications · 849 citations

    12

    h-index

  2. AG
    Andrew Gould

    The Ohio State University, United States

    12 publications · 685 citations

    12

    h-index

  3. CH
    Cheongho Han

    Chungbuk National University, South Korea

    10 publications · 289 citations

    10

    h-index

  4. MK
    M. K. Szymański

    University of Warsaw, Poland

    12 publications · 622 citations

    10

    h-index

  5. IS
    I. Soszyński

    University of Warsaw, Poland

    12 publications · 622 citations

    10

    h-index

1–5 of 415

Venues

  1. The Astrophysical Journal

    ApJ · 42 publications · 2.4K citations

    30

    h-index

  2. 15

    h-index

  3. The Astrophysical Journal Letters

    4 publications · 225 citations

    4

    h-index

  4. CERN Document Server (European Organization for Nuclear Research)

    Repository · 4 publications · 62 citations

    4

    h-index

  5. ArXiv.org

    Repository · 3 publications · 43 citations

    3

    h-index

1–5