Abstract The Kepler Mission is a space observatory launched in 2009 by NASA to monitor
170 000 stars over a period of four years to determine the frequency of Earth-size and larger …

The detection of exoplanets orbiting other stars has revolutionized our view of the cosmos.
First results suggest that it is teeming with a fascinating diversity of rocky planets, including …

We present 2241 exoplanet candidates identified with data from the Transiting Exoplanet
Survey Satellite (TESS) during its 2 yr Prime Mission. We list these candidates in the TESS …

Abstract NASA's Kepler Space Telescope was designed to determine the frequency of Earth-
sized planets orbiting Sun-like stars, but these planets are on the very edge of the mission's …

The population of planets smaller than approximately 1.7 Earth radii (R⊕) is widely
interpreted as consisting of rocky worlds, generally referred to as super-Earths. This picture …

This paper discusses the transit model-fitting and multiple-planet search algorithms and
performance of the Kepler Science Data Processing Pipeline, developed by the Kepler …

We present an improved estimate of the occurrence rate of small planets orbiting small stars
by searching the full four-year Kepler data set for transiting planets using our own planet …

We present astrophysical false positive probability calculations for every Kepler Object of
Interest (KOI)—the first large-scale demonstration of a fully automated transiting planet …

We have established precise planet radii, semimajor axes, incident stellar fluxes, and stellar
masses for 909 planets in 355 multi-planet systems discovered by Kepler. In this sample, we …

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing
accurate key planet parameters (radius, mass, density and age) in statistical numbers, it …