Geometric Parallax
Geometric Parallax is a measurement method in astrometry that determines the distance to a celestial object by observing its apparent shift in position relative to background stars from two distinct vantage points, using the principles of triangulation.
65
Publications
4.5K
Citations
181
Authors
103
Institutions
Publications per year
2017–2026
16
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103
Swinburne University of Technology
Melbourne, Australia
4 h-index
9 publications
211 citations

Johns Hopkins University Applied Physics Laboratory
North Laurel, United States
4 h-index
10 publications
308 citations

Cornell University
Ithaca, United States
3 h-index
3 publications
73 citations
Curtin University
Perth, Australia
3 h-index
4 publications
790 citations

York University
Toronto, Canada
2 h-index
2 publications
59 citations
Arcetri Astrophysical Observatory
Florence, Italy
2 h-index
2 publications
163 citations
Northwestern University
Evanston, United States
2 h-index
8 publications
94 citations
National Radio Astronomy Observatory
Charlottesville, United States
2 h-index
2 publications
71 citations
1–8 of 103
ApJ · 7 publications · 406 citations
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4 publications · 195 citations
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AJ · 4 publications · 2K citations
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JHA · 2 publications · 44 citations
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2 publications · 78 citations
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