Not exact matches
The data on the numerous
candidates are somewhat preliminary and
require validation, but a new analysis by a pair of astrophysicists at the California Institute of Technology suggests that the percentage of false positives among Kepler's
candidate planets may be less than 10 percent.
The lower abundance of diluted binaries between 0.1 and 0.4 % transit depth, which possibly continues towards lower - amplitude
candidates, may facilitate the transit - searches for small extrasolar
planets in both CoRoT data and in upcoming or planned search projects, such as Kepler or PLATO, reducing the load of
required follow - up observations.
Candidates require follow - up observations and analysis to verify they are actual
planets.
Comparing our sample to the Kepler
candidate sample investigated by Fulton et al. (2017), we conclude that more
planets are
required to quantitatively confirm the gap with K2
candidates or validated
planets.