C-19 stellar stream members from this work. The declination vs radial velocity distribution (top) and declination vs right ascension distribution (bottom) of the INT sample of V/EMP stars are colour-coded by their inferred spectroscopic metallicities with the C-19 orbit from the STREAMFINDER algorithm and the Yuan et al. (2022) identified C-19 members overlaid. The tentative C-19 members identified in this work are shown as large star markers. All EMP stars observable by the spectroscopic follow-up program at INT are shown in grey.