Reference Star Selection
Reference Star Selection is the systematic process of identifying and choosing stable, well-characterized stars within a field of view to serve as positional fiducials in differential astrometry, distinguished by their photometric stability, astrometric precision, and spatial distribution relative to the target object.
46
Publications
2.4K
Citations
247
Authors
157
Institutions
Publications per year
2017–2026
14
46
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
<i>Gaia</i>FGK benchmark stars: Metallicity
P. Jofré, U. Heiter, C. Soubiran et al. · Astronomy and Astrophysics · 2014 · 313 citations · Full text
Natural Sciences, Astronomy, Physics +17
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157

Centre National de la Recherche Scientifique
Paris, France
8 h-index
43 publications
3.6K citations
Délégation Paris 7
Bagnolet, France
5 h-index
16 publications
502 citations
European Southern Observatory
Santiago, Chile
5 h-index
12 publications
588 citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
5 h-index
16 publications
539 citations

Space Telescope Science Institute
Baltimore, United States
5 h-index
10 publications
276 citations
Université Paris Cité
Paris, France
4 h-index
13 publications
323 citations

Sorbonne Université
Paris, France
4 h-index
9 publications
219 citations
United States Naval Observatory
Flagstaff, United States
4 h-index
5 publications
423 citations
1–8 of 157
AJ · 8 publications · 297 citations
8
h-index
8 publications · 572 citations
8
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5 publications · 200 citations
5
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4 publications · 154 citations
4
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1 publications · 24 citations
1
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