A possible third body in the X-ray system GRS 1747−312 and models with higher order multiplicity
C. A. Painter(Center for Astrophysics Harvard & Smithsonian), Hideyuki Mori(Japan Aerospace Exploration Agency), Roberto Soria, Ryan Urquhart(Curtin University), Darin Ragozzine(Brigham Young University), V. Kashyap(Center for Astrophysics Harvard & Smithsonian), R. Di Stefano(Center for Astrophysics Harvard & Smithsonian), J. López-Miralles(European Space Astronomy Centre), James F. Steiner(Center for Astrophysics Harvard & Smithsonian), S. Motta(Brera Astronomical Observatory)
Cited by 8
Related Papers
PLANETARY CANDIDATES OBSERVED BY <i>KEPLER</i> . III. ANALYSIS OF THE FIRST 16 MONTHS OF DATA
|The Astrophysical Journal Supplement Series|2013|1.1k
Statistics, Handle with Care: Detecting Multiple Model Components with the Likelihood Ratio Test
|The Astrophysical Journal|2002|696
Transiting circumbinary planets Kepler-34 b and Kepler-35 b
|Nature|2012|485
KEPLER ECLIPSING BINARY STARS. VII. THE CATALOG OF ECLIPSING BINARIES FOUND IN THE ENTIRE KEPLER DATA SET
|The Astronomical Journal|2016|441
Kepler-47: A Transiting Circumbinary Multiplanet System
|Science|2012|380