The Pristine survey - VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates

none30siWe present the results of a 3-yr long, medium-resolution spectroscopic campaign aimed at identifying very metal-poor stars from candidates selected with the CaHK, metallicity-sensitive Pristine survey. The catalogue consists of a total of 1007 stars, and includes 146 rediscoveries of metal-poor stars already presented in previous surveys, 707 new very metal-poor stars with [Fe/H] < −2.0, and 95 new extremely metal-poor stars with [Fe/H] < −3.0. We provide a spectroscopic [Fe/H] for every star in the catalogue, and [C/Fe] measurements for a subset of the stars (10 per cent with [Fe/H] < −3 and 24 per cent with −3 < [Fe/H] < −2) for which a carbon determination is possible, contingent mainly on the carbon abundance, effective temperature and signal-to-noise ratio of the stellar spectra. We find an average carbon enhancement fraction ([C/Fe] ≥ +0.7) of 41 ± 4 per cent for stars with −3 < [Fe/H] < −2 and 58 ± 14 per cent for stars with [Fe/H] < −3, and report updated success rates for the Pristine survey of 56 per cent and 23 per cent to recover stars with [Fe/H] < −2.5 and < −3, respectively. Finally, we discuss the current status of the survey and its preparation for providing targets to upcoming multi-object spectroscopic surveys such as William Herschel Telescope Enhanced Area Velocity Explorer.openAguado D.S.; Youakim K.; Gonzalez Hernandez J.I.; Prieto C.A.; Starkenburg E.; Martin N.; Bonifacio P.; Arentsen A.; Caffau E.; de Arriba L.P.; Sestito F.; Garcia-Dias R.; Fantin N.; Hill V.; Jablonca P.; Jahandar F.; Kielty C.; Longeard N.; Lucchesi R.; Sanchez-Janssen R.; Osorio Y.; Palicio P.A.; Tolstoy E.; Wilson T.G.; Cote P.; Kordopatis G.; Lardo C.; Navarro J.F.; Thomas G.F.; Venn K.Aguado D.S.; Youakim K.; Gonzalez Hernandez J.I.; Prieto C.A.; Starkenburg E.; Martin N.; Bonifacio P.; Arentsen A.; Caffau E.; de Arriba L.P.; Sestito F.; Garcia-Dias R.; Fantin N.; Hill V.; Jablonca P.; Jahandar F.; Kielty C.; Longeard N.; Lucchesi R.; Sanchez-Janssen R.; Osorio Y.; Palicio P.A.; Tolstoy E.; Wilson T.G.; Cote P.; Kordopatis G.; Lardo C.; Navarro J.F.; Thomas G.F.; Venn K