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
Parents
95
M. A. Walker · The Astrophysical Journal · 1995 · 199 citations
Natural Sciences, Astronomy, Physics +16
Astrometry for Determining the MACHO Mass and Trajectory
M. Miyamoto, Yuzuru Yoshi · The Astronomical Journal · 1995 · 166 citations · Full text
Natural Sciences, Astronomy, Physics +16
Astrometric Microlensing of Stars
M. Dominik, K. C. Sahu · The Astrophysical Journal · 2000 · 165 citations
Natural Sciences, Astronomy, Physics +16
Measuring the Remnant Mass Function of the Galactic Bulge
Andrew Gould · The Astrophysical Journal · 2000 · 156 citations · Full text
Natural Sciences, Astronomy, Physics +14
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199
The Ohio State University
Columbus, United States
17 h-index
47 publications
2.2K citations

University of Warsaw
Warsaw, Poland
13 h-index
104 publications
6.6K citations

Chungbuk National University
Cheongju-si, South Korea
12 h-index
24 publications
668 citations

Space Telescope Science Institute
Baltimore, United States
12 h-index
52 publications
3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
8 h-index
9 publications
326 citations
Université Bourgogne Franche-Comté
Besançon, France
8 h-index
30 publications
2K citations
California Institute of Technology
Pasadena, United States
8 h-index
19 publications
548 citations
Princeton University
Princeton, United States
7 h-index
8 publications
596 citations
1–8 of 199
ApJ · 42 publications · 2.4K citations
30
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16 publications · 729 citations
15
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4 publications · 225 citations
4
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Repository · 4 publications · 62 citations
4
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Repository · 3 publications · 43 citations
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