gt; -0.75$) of halo stars located at distances from the Galactic plane $z$ up to $|z| \sim 10$ kpc, observed by the Apache Point Observatory Galactic Evolution Experiment (APOGEE). We examine the chemistry, kinematics, and dynamics of this metal-r…" /> The metal-rich halo tail extended in |z|: a characterization with Gaia DR2 and APOGEE