Sidereal Observations
Sidereal Observations is a systematic method in astronomical surveying that measures the positions and motions of celestial objects relative to distant stars, distinguished by its use of sidereal time and inertial reference frames fixed with respect to the celestial sphere.
114
Publications
6.5K
Citations
2.6K
Authors
484
Institutions
Publications per year
2017–2026
15
Parents
114
The period and Q of the Chandler wobble
Melvyn Smith, F. A. Dahlen · Geophysical Journal International · 1981 · 308 citations
1–5 of 114
2.6K
Center for Astrophysics Harvard & Smithsonian, United States
4 publications · 718 citations
4
h-index
3
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3
h-index
Center for Astrophysics Harvard & Smithsonian, United States
3 publications · 415 citations
3
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3
h-index
1–5 of 2.6K
484
University of Arizona
Tucson, United States
7 h-index
17 publications
931 citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
125 publications
12.5K citations
Indiana University Bloomington
Bloomington, United States
6 h-index
19 publications
2.2K citations

Kyoto University
Kyoto, Japan
5 h-index
38 publications
2.7K citations
Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
Rome, Italy
5 h-index
36 publications
3.4K citations

Chinese Academy of Sciences
Beijing, China
5 h-index
109 publications
22.4K citations

University of Rome Tor Vergata
Rome, Italy
4 h-index
19 publications
1.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
30 publications
5K citations
1–8 of 484
7 publications · 768 citations
7
h-index
PRL · 7 publications · 771 citations
7
h-index
AJ · 7 publications · 230 citations
7
h-index
PRD · 6 publications · 319 citations
6
h-index
ApJ · 6 publications · 428 citations
6
h-index
1–5