Binary Star Light Curves
Binary Star Light Curves is a time-series photometric measurement that represents the changes in apparent brightness of a binary star system over time due to mutual eclipses, orbital motions, and irradiation effects intrinsic to the system’s geometry and stellar components.
916
Publications
40.7K
Citations
2.4K
Authors
705
Institutions
Publications per year
2017–2026
125
916
New limb-darkening coefficients for modeling binary star light curves
W. Van Hamme · The Astronomical Journal · 1993 · 1.5K citations
Natural Sciences, Astronomy, Physics +10
Period determination using phase dispersion minimization
R. F. Stellingwerf · The Astrophysical Journal · 1978 · 1.5K citations
Natural Sciences, Astronomy, Physics +13
1–5 of 916
2.4K
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705
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
31 h-index
80 publications
5.8K citations

Chinese Academy of Sciences
Beijing, China
29 h-index
293 publications
9.2K citations
California Institute of Technology
Pasadena, United States
26 h-index
91 publications
9.6K citations
National Astronomical Observatories
Beijing, China
25 h-index
185 publications
6.3K citations

Korea Astronomy and Space Science Institute
Daejeon, South Korea
22 h-index
183 publications
4.9K citations

Space Telescope Science Institute
Baltimore, United States
21 h-index
28 publications
2.1K citations

Centre National de la Recherche Scientifique
Paris, France
21 h-index
57 publications
3K citations

Keele University
Newcastle-under-Lyme, United Kingdom
21 h-index
42 publications
2.9K citations
1–8 of 705
ApJ · 180 publications · 11.9K citations
54
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169 publications · 7.4K citations
45
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AJ · 171 publications · 8K citations
42
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108 publications · 4.9K citations
32
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PASP · 52 publications · 1.8K citations
22
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