Photometric Binaries
Photometric Binaries is a class of binary star systems identified and characterized by periodic variations in their observed brightness, arising from mutual eclipses or distortions in their shapes due to gravitational interaction, detectable through photometric measurements without requiring direct spectral or positional resolution.
619
Publications
28.7K
Citations
2K
Authors
677
Institutions
Publications per year
2017–2026
99
Parents
619
THE FALSE POSITIVE RATE OF<i>KEPLER</i>AND THE OCCURRENCE OF PLANETS
The Astrophysical Journal · 2013 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +14
Cygnus X-1—a Spectroscopic Binary with a Heavy Companion ?
B. L. Webster, Paul Murdin · Nature · 1972 · 476 citations
Natural Sciences, Astronomy, Physics +15
1–5 of 619
2K
21
h-index
16
h-index
16
h-index
13
h-index
12
h-index
1–5 of 2K
677

Chinese Academy of Sciences
Beijing, China
28 h-index
269 publications
8.4K citations
National Astronomical Observatories
Beijing, China
25 h-index
191 publications
6.4K citations

Space Telescope Science Institute
Baltimore, United States
24 h-index
45 publications
4.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
23 h-index
58 publications
2K citations
California Institute of Technology
Pasadena, United States
22 h-index
94 publications
4.7K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
21 h-index
50 publications
2.6K citations

Yunnan Observatories
Kunming, China
20 h-index
152 publications
4K citations

Centre National de la Recherche Scientifique
Paris, France
20 h-index
79 publications
3K citations
1–8 of 677
ApJ · 103 publications · 8.3K citations
43
h-index
AJ · 121 publications · 5.1K citations
37
h-index
85 publications · 4K citations
36
h-index
103 publications · 3.8K citations
36
h-index
PASP · 20 publications · 497 citations
16
h-index
1–5