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- W3130010206 abstract "Over 4,000 exoplanets have been identified and thousands of candidates are to be confirmed. The relations between the characteristics of these planetary systems and the kinematics, Galactic components, and ages of their host stars have yet to be well explored. Aiming to addressing these questions, we conduct a research project, dubbed as PAST (Planets Across Space and Time). To do this, one of the key steps is to accurately characterize the planet host stars. In this paper, the Paper I of the PAST series, we revisit the kinematic method for classification of Galactic components and extend the applicable range of velocity ellipsoid from about 100 pc to 1, 500 pc from the sun in order to cover most known planet hosts. Furthermore, we revisit the Age-Velocity dispersion Relation (AVR), which allows us to derive kinematic age with a typical uncertainty of 10-20% for an ensemble of stars. Applying the above revised methods, we present a catalog of kinematic properties (i.e. Galactic positions, velocities, the relative membership probabilities among the thin disk, thick disk, Hercules stream, and the halo) as well as other basic stellar parameters for 2,174 host stars of 2,872 planets by combining data from Gaia, LAMOST, APOGEE, RAVE, and the NASA exoplanet archive. The revised kinematic method and AVR as well as the stellar catalog of kinematic properties and ages lay foundation for future studies on exoplanets from two dimensions of space and time in the Galactic context." @default.
- W3130010206 created "2021-03-01" @default.
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- W3130010206 date "2021-03-01" @default.
- W3130010206 modified "2023-09-29" @default.
- W3130010206 title "Planets Across Space and Time (PAST). I. Characterizing the Memberships of Galactic Components and Stellar Ages: Revisiting the Kinematic Methods and Applying to Planet Host Stars" @default.
- W3130010206 cites W147232447 @default.
- W3130010206 cites W1922052071 @default.
- W3130010206 cites W1965209244 @default.
- W3130010206 cites W1972506885 @default.
- W3130010206 cites W1979379324 @default.
- W3130010206 cites W1983114381 @default.
- W3130010206 cites W1986099565 @default.
- W3130010206 cites W1991655134 @default.
- W3130010206 cites W1998084400 @default.
- W3130010206 cites W1999894587 @default.
- W3130010206 cites W2016734711 @default.
- W3130010206 cites W2025070354 @default.
- W3130010206 cites W2028070372 @default.
- W3130010206 cites W2033393106 @default.
- W3130010206 cites W2035525551 @default.
- W3130010206 cites W2039406483 @default.
- W3130010206 cites W2059104746 @default.
- W3130010206 cites W2063151445 @default.
- W3130010206 cites W2067530731 @default.
- W3130010206 cites W2068903138 @default.
- W3130010206 cites W2069495360 @default.
- W3130010206 cites W2072195551 @default.
- W3130010206 cites W2072610194 @default.
- W3130010206 cites W2089014417 @default.
- W3130010206 cites W2100833883 @default.
- W3130010206 cites W2100893534 @default.
- W3130010206 cites W2103367868 @default.
- W3130010206 cites W2109032933 @default.
- W3130010206 cites W2128653677 @default.
- W3130010206 cites W2132514858 @default.
- W3130010206 cites W2133725650 @default.
- W3130010206 cites W2136396438 @default.
- W3130010206 cites W2136484893 @default.
- W3130010206 cites W2155457133 @default.
- W3130010206 cites W2155488926 @default.
- W3130010206 cites W2169344843 @default.
- W3130010206 cites W2174591450 @default.
- W3130010206 cites W2206917439 @default.
- W3130010206 cites W2268645779 @default.
- W3130010206 cites W2276916864 @default.
- W3130010206 cites W2463543304 @default.
- W3130010206 cites W2558422827 @default.
- W3130010206 cites W2578206578 @default.
- W3130010206 cites W2581895953 @default.
- W3130010206 cites W2609118998 @default.
- W3130010206 cites W2775275747 @default.
- W3130010206 cites W2781275565 @default.
- W3130010206 cites W2798158223 @default.
- W3130010206 cites W2798336535 @default.
- W3130010206 cites W2911118502 @default.
- W3130010206 cites W2913667320 @default.
- W3130010206 cites W2938416494 @default.
- W3130010206 cites W2948218282 @default.
- W3130010206 cites W2948879413 @default.
- W3130010206 cites W2963974970 @default.
- W3130010206 cites W2971748990 @default.
- W3130010206 cites W2974366455 @default.
- W3130010206 cites W3028685339 @default.
- W3130010206 cites W3032874046 @default.
- W3130010206 cites W3098830536 @default.
- W3130010206 cites W3098867955 @default.
- W3130010206 cites W3099338766 @default.
- W3130010206 cites W3099823360 @default.
- W3130010206 cites W3099975694 @default.
- W3130010206 cites W3100601934 @default.
- W3130010206 cites W3100835200 @default.
- W3130010206 cites W3102030042 @default.
- W3130010206 cites W3102087921 @default.
- W3130010206 cites W3102850733 @default.
- W3130010206 cites W3102986170 @default.
- W3130010206 cites W3103009155 @default.
- W3130010206 cites W3103263672 @default.
- W3130010206 cites W3103390308 @default.
- W3130010206 cites W3103639866 @default.
- W3130010206 cites W3103997796 @default.
- W3130010206 cites W3104487947 @default.
- W3130010206 cites W3104489242 @default.
- W3130010206 cites W3104493829 @default.
- W3130010206 cites W3105292504 @default.
- W3130010206 cites W3105904302 @default.
- W3130010206 cites W3106294757 @default.
- W3130010206 cites W3124275756 @default.
- W3130010206 cites W3125696588 @default.