Left panel: distribution of Psc-Eri stars from the 3NB sample (see Sect. 2.2) shown as blue dots in the tangential velocity plane ΔV_∥, ΔV_⊥ and see text for further explanation). The yellow dots represent a subset of the 3NB sample within a radius of 2.5 km s⁻¹ around the origin. The Meingast et al. (2019) stars found in our 3NB sample are marked by black dots. Middle and right panels: distribution of stream candidates in the Y, X plane and the X, Z plane. The cyan dots show the final sample of the Psc-Eri stream. The yellow and black dots represent the same data as in the left panel.