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The Kepler telescope has discovered over 4,000 planets (candidates) bysearching ? 200,000 stars over a wide range of distance (order of kpc) in ourGalaxy. Characterizing the kinematic properties (e.g., Galactic componentmembership and kinematic age) of these Kepler targets (including the planet(candidate) hosts) is the first step towards studying Kepler planets in theGalactic context, which will reveal fresh insights into planet formation andevolution. In this paper, the second part of the Planets Across the Space andTime (PAST) series, by combining the data from LAMOST and Gaia and thenapplying the revised kinematic methods from PAST I, we present a catalog ofkinematic properties(i.e., Galactic positions, velocities, and the relativemembership probabilities among the thin disk, thick disk, Hercules stream, andthe halo) as well as other basic stellar parameters for 35,835 Kepler stars.Further analyses of the LAMOST-Gaia-Kepler catalog demonstrate that our derivedkinematic age reveals the expected stellar activity-age trend. Furthermore, wefind that the fraction of thin(thick) disk stars increases (decreases) with thetransiting planet multiplicity (Np = 0, 1, 2 and 3+) and the kinematic agedecreases with Np, which could be a consequence of the dynamical evolution ofplanetary architecture with age. The LAMOST-Gaia-Kepler catalog will be usefulfor future studies on the correlations between the exoplanet distributions andthe stellar Galactic environments as well as ages.

Planets Across Space and Time (PAST). II: Catalog and Analyses of the LAMOST-Gaia-Kepler Stellar Kinematic Properties