Reference Frame Transformations
Reference Frame Transformations is a formal method in astrometry that specifies the mathematical procedures and kinematic models required to convert positional and rotational measurements from one celestial or terrestrial reference frame to another, accounting for time-dependent effects such as Earth rotation, polar motion, and relativistic frame-dragging.
188
Publications
11K
Citations
414
Authors
225
Institutions
Publications per year
2017–2026
44
188
1–5 of 188
414
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225
Jet Propulsion Laboratory
Pasadena, United States
7 h-index
8 publications
274 citations
Institute of Applied Astronomy
Saint Petersburg, Russia
5 h-index
5 publications
251 citations
NOAA National Geodetic Survey
Silver Spring, United States
5 h-index
10 publications
288 citations
University of Vienna
Vienna, Austria
4 h-index
10 publications
1.6K citations
Vienna Center for Quantum Science and Technology
Vienna, Austria
4 h-index
11 publications
1.7K citations
Austrian Academy of Sciences
Vienna, Austria
4 h-index
10 publications
1.4K citations

Perimeter Institute
Waterloo, Canada
4 h-index
5 publications
234 citations
ETH Zurich
Zurich, Switzerland
4 h-index
8 publications
1.8K citations
1–8 of 225
6 publications · 471 citations
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PRD · 6 publications · 194 citations
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5 publications · 220 citations
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5 publications · 110 citations
5
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5 publications · 225 citations
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