A catalogue of asteroseismically calibrated ages for APOGEE DR17 - The predictions of a CatBoost machine learning model based on the [Mg/Ce] chemical clock and other stellar parameters

Open Access

Table E.3

Kinematic properties pertaining to the second group of young metal-poor stars. The parameters are the same as in Table E.1.

Gaia DR3	U(LSR)	V(LSR)	W(LSR)	e	P	Group

	km/s	km/s	km/s	$0$ $\cancel{0}$	$0$ $\cancel{0}$	$0$ $\cancel{0}$
5413585519599048448	306.988	−427.339	168.863	0.825	1.000	halo
5413576860944908416	297.867	−427.592	156.149	0.788	1.000	halo
5413576689146193280	314.877	−426.684	167.581	0.84	1.000	halo
5413574073501926528	302.783	−435.287	156.194	0.812	1.000	halo
5413575344812320640	343.661	−418.231	185.970	0.91	1.000	halo

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