The majority of exoplanet discoveries in 2016 were from a paper by Morton et al. that statistically validated over 1,000 Kepler planets.[61] This statistical validation did not involve mass measurements, and some transiting objects validated as planets were later shown (or even previously known) to be small stars. Such cases include Kepler-469 (KOI-126),[96] Kepler-470 (KOI-129),[97] Kepler-486 (KOI-189),[98] Kepler-488 (KOI-194),[99] Kepler-503 (KOI-242),[100] Kepler-628 (KOI-631),[101] Kepler-699 (KOI-846),[63] Kepler-706 (KOI-855),[101] Kepler-807 (KOI-1288),[101] Kepler-840 (KOI-1416),[63] and Kepler-854 (KOI-1450).[63] In another two cases, Kepler-492 (KOI-205)[102] and Kepler-494 (KOI-219),[101] the companions are brown dwarfs with masses about 40 times that of Jupiter.
HD 131399 Ab had been thought to be a massive directly-imaged planet located in a trinary system. Later analysis showed that it is a background star instead.[103]
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