Pascale Jablonka, Willem Suter, Carmela Lardo, Romain Ely Roland Lucchesi
We present a one-dimensional, local thermodynamic equilibrium homogeneous analysis of 132 stars observed at high resolution with ESPaDOnS. This represents the largest sample observed at high resolution (R similar to 40 000) from the Pristine survey. This sample is based on the first version of the Pristine catalogue and covers the full range of metallicities from [Fe/II] similar to-3 to similar to+0.25, with nearly half of our sample (58 stars) composed of very metal-poor (VMP) stars ([Fe/H]
OXFORD UNIV PRESS2022