Surface Gravity Determination
Surface Gravity Determination is a spectroscopic method in stellar astrophysics that infers the gravitational acceleration at a star's photosphere by analyzing pressure-sensitive spectral line broadening and ionization equilibria, distinguishing it from other stellar parameter estimation techniques through its specific sensitivity to surface gravity effects on spectral features.
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Deformation induced by polar motion
John Wahr · Journal of Geophysical Research Atmospheres · 1985 · 344 citations
SELECTION, PRIORITIZATION, AND CHARACTERISTICS OF <i>KEPLER</i> TARGET STARS
Natalie M. Batalha, W. J. Borucki, David Koch et al. · The Astrophysical Journal Letters · 2010 · 316 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Centre National de la Recherche Scientifique
Paris, France
22 h-index
87 publications
6.1K citations
University of Arizona
Tucson, United States
15 h-index
24 publications
2.3K citations
Université Paris Cité
Paris, France
13 h-index
29 publications
1.6K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
13 h-index
23 publications
1.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
12 h-index
33 publications
3.1K citations
The University of Texas at Austin
Austin, United States
12 h-index
24 publications
941 citations
Délégation Paris 7
Bagnolet, France
12 h-index
18 publications
1.1K citations

Ames Research Center
Mountain View, United States
11 h-index
20 publications
2.3K citations
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ApJ · 46 publications · 3.1K citations
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27 publications · 1.9K citations
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31 publications · 1.6K citations
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AJ · 11 publications · 549 citations
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10 publications · 677 citations
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