The missions

Kepler & K2 provide long-baseline, high-precision photometry for exoplanet and astrophysics research.

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K2 observing

K2 is a community-driven mission: targets and funding are awarded through open calls for proposals.

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Data analysis

Pixel data, lightcurves, and analysis software are publicly available with no proprietary period.

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News for scientists



K2 Campaign 5 reprocessed

Earlier this year we announced that we were undertaking an effort to reprocess campaigns 0–14 using the same version of the Kepler/K2 pipeline used for C15 and subsequent campaigns. This version introduced several new features and improvements, such as more sophisticated pixel calibration, better identification of spacecraft pointing …

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K2 Campaign 0 reprocessed

Earlier this year we announced that we were undertaking an effort to reprocess campaigns 0–14 using the same version of the Kepler/K2 pipeline used for C15 and subsequent campaigns. This version introduced several new features and improvements, such as more sophisticated pixel calibration, better identification of spacecraft pointing …

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New white paper: Scientific Opportunities with Kepler & K2 Archive Data

The Kepler and K2 missions have provided an unprecedented data set with a precision and duration that will not be rivaled for decades. Even though the data has already contributed to nearly 2,500 scientific publications so far, the scientific community continues to extract new discoveries from the archive data …

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New in Lightkurve: the Periodogram class

This month in Lightkurve, we have added a Periodogram class, which provides a quick and easy way to create Lomb-Scargle periodograms from LightCurve objects.

Periodograms can be used to find stellar rotation rates, or the oscillation and pulsation frequencies of stars. They are commonly used in asteroseismology to identify oscillation …

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