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The Low-$α$ Splash Population in the Milky Way
The Milky Way in-situ halo, also known as the Splash, consists of old (age $>$ 10 Gyr), metal-rich ([Fe/H] $> -0.7$), high-$α$ stars, i.e., thick disk-like chemistry, on halo-like orbits (eccentricity $>$ 0.6). Its origin is linked to stars formed in the disk and dynamically heated by either interna
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