Exploring the Compositional Diversity of Small Exoplanets from K2
This Keck Science Mission Support project (PI: A. Howard) observed a large collection of stars hosting super-Earths and Neptune-size planets discovered by the K2 mission extension to Kepler. The project has contributed radial velocities, activity indicators, and derived stellar properties for their sample of stars.
- Table and Data of 2332 RV and Activity measurements for 84 stars.
- Table and Data of Derived Properties for 440 Stars
Please acknowledge the use of KOA by including this text in your publications:
This research has made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration.
Please also acknowledge the PI(s) of datasets that have been obtained through KOA, and please contact the KOA Help Desk if you publish archival data.
If your research uses data reduced by the DEIMOS DRP or MOSFIRE DRP, please use the PypeIt Citation.
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The Keck Observatory Archive (KOA) is a collaboration between the NASA Exoplanet Science Institute (NExScI) and the W. M. Keck Observatory (WMKO). NExScI is sponsored by NASA's Exoplanet Exploration Program, and operated by the California Institute of Technology in coordination with the Jet Propulsion Laboratory (JPL).
