The California-Kepler Survey. VI: Kepler Multis and Singles Have Similar Planet and Stellar Properties Indicating a Common Origin
Lauren M. Weiss, Howard T. Isaacson, Geoffrey W. Marcy, Andrew W., Howard, Erik A. Petigura, Benjamin J. Fulton, Joshua N. Winn, Lea Hirsch,, Evan Sinukoff, Jason F. Rowe

TL;DR
This study finds that single and multi-planet systems detected by Kepler share similar stellar and planetary properties, implying a common origin, with differences mainly in short-period planets likely due to dynamical evolution.
Contribution
It provides evidence that singles and multis have similar properties, supporting the idea of a shared origin and possible planet-planet scattering in singles.
Findings
Singles and multis have indistinguishable stellar properties.
Both show a similar radius valley at ~1.8 R_⊕.
More short-period singles suggest dynamical evolution effects.
Abstract
The California-Kepler Survey (CKS) catalog contains precise stellar and planetary properties for the \Kepler\ planet candidates, including systems with multiple detected transiting planets ("multis") and systems with just one detected transiting planet ("singles," although additional planets could exist). We compared the stellar and planetary properties of the multis and singles in a homogenous subset of the full CKS-Gaia catalog. We found that sub-Neptune sized singles and multis do not differ in their stellar properties or planet radii. In particular: (1.) The distributions of stellar properties , [Fe/H], and for the Kepler sub Neptune-sized singles and multis are statistically indistinguishable. (2.) The radius distributions of the sub-Neptune sized singles and multis with days are indistinguishable, and both have a valley at .…
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