1. Introduction

2. Target Selection  
2.1. The Pristine survey and success rates  
2.2. Pristine-Gaia synthetic catalogue of photometric metallicities  

3. INT/IDS spectroscopic follow-up of V/EMP candidates  
3.1. Data reduction  
3.2. Radial velocities  
3.3. Metallicities  

4. Results  
4.1. Performance of the Pristine-Gaia synthetic pre-selection  
4.2. Chemo kinematics of the V/EMP stars  

5. Discussion  
5.1. Planar metal-poor stars  
5.2. C-19 stellar stream new members  

6. Conclusions and Outlook