11 Dec 2010: The time of secondary eclipse is not measured but derived from the Keplerian orbit (Bakos et al. 2010).
31 Jul 2024.: See also Planets in Binaries webpage.
Search for Stellar Companions of Exoplanet Host Stars with AstraLux/CAHA 2.2 m
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Gaia Search for (sub)stellar Companions of Exoplanet Hosts
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Planetary Parameters, XUV Environments, and Mass-loss Rates for Nearby Gaseous Planets with X-Ray-detected Host Stars
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The GAPS Programme with HARPS-N at TNG. XIII. The orbital obliquity of three close-in massive planets hosted by dwarf K-type stars: WASP-43, HAT-P-20 and Qatar-2
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Defocused Observations of Selected Exoplanet Transits with T100 in TUBITAK National Observatory of Turkey (TUG)
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in "Living Together: Planets, Host Stars and Binaries " Litomysi 2015
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Spitzer Secondary Eclipses of the Dense, Modestly-irradiated, Giant Exoplanet HAT-P-20b Using Pixel-level Decorrelation
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Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-period Companions to Close-in Gas Giant Planets
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Factors Affecting the Radii of Close-in Transiting Exoplanets
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Constraining Tidal Dissipation in Stars from The Destruction Rates of Exoplanets
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