Stellar Distance Determination
Stellar Distance Determination is a methodological framework in astrophysics that systematically quantifies the spatial separation between celestial observers and stars through the application of geometric, photometric, or spectroscopic principles to observed astronomical data.
1.3K
Publications
92.3K
Citations
3.6K
Authors
845
Institutions
Publications per year
2017–2026
252
Parents
1.3K
MONITORING STELLAR ORBITS AROUND THE MASSIVE BLACK HOLE IN THE GALACTIC CENTER
S. Gillessen, F. Eisenhauer, Sascha Trippe et al. · The Astrophysical Journal · 2009 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 1.3K
3.6K
Laboratoire d’études spatiales et d’instrumentation en astrophysique, France
31 publications · 1.8K citations
25
h-index
23
h-index
20
h-index
19
h-index
18
h-index
1–5 of 3.6K
845

Centre National de la Recherche Scientifique
Paris, France
54 h-index
719 publications
118.5K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
46 h-index
189 publications
39K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
44 h-index
161 publications
32K citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
39 h-index
139 publications
18.5K citations
California Institute of Technology
Pasadena, United States
39 h-index
105 publications
7.7K citations

Space Telescope Science Institute
Baltimore, United States
38 h-index
117 publications
17.6K citations
Carnegie Observatories
Pasadena, United States
36 h-index
124 publications
14.2K citations

Observatoire de Paris
Paris, France
35 h-index
152 publications
34.7K citations
1–8 of 845
ApJ · 344 publications · 30.2K citations
89
h-index
212 publications · 18.1K citations
64
h-index
197 publications · 10.1K citations
57
h-index
AJ · 171 publications · 14K citations
55
h-index
Repository · 21 publications · 1.2K citations
19
h-index
1–5