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Stellar surface inhomogeneities as a potential source of the atmospheric signal detected in the K2-18 b transmission spectrum
Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months)
Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set
Planetary candidates observed by Kepler. VI. Planet sample from Q1--Q16 (47 months)
Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data
A class of eccentric binaries with dynamic tidal distortions discovered with Kepler
The NASA GSFC TESS Full Frame Image Light Curve Data Set
The transmission spectrum of the potentially rocky planet L 98-59 c
L 98-59: A Benchmark System of Small Planets for Future Atmospheric Characterization
Kepler eclipsing binary stars. III. Classification of Kepler eclipsing binary light curves with locally linear embedding
