Fig. 7

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Distribution of low-metallicity stars from the INT sample in the Jϕ−Jɀ action space. The action quantities are scaled by the solar values (i.e., Jϕ⊙ = 2009.92 kpc km/s, Jɀ⊙ = 0.35 kpc km/s). The two black boxes represent the prograde and the retrograde disc-like orbits showing an overdensity in the prograde direction. All EMP stars observable by the spectroscopic follow-up program at INT are shown in grey.
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