• MINCE – Measuring at Intermediate Metallicity Neutron-Capture Elements (Cescutti)– observations have been conducted and the analysis is ongoing. Observations have been/are to be carried out with:
  1. CFHT (Bonifacio),
  2. VLT/UVES, TNG/HARPS-N (Cescutti),
  3. 2/FEROS (Hansen).
  4. VUES/Moletai (Kučinskas)

• r-process in Extremely Metal-Poor stars – using VLT/UVES+X-Shooter (Hansen). The observations were stalled and carried over to this observing period and then unfortunately delayed.

• “Bafnium” – VLT/UVES (Hansen). The data reduction is ongoing and the analysis will start soon.

• Be in globular clusters – VLT/UVES (Kučinskas). Observations granted – may be carried over to next period.

Some observations were cancelled or carried over to the following period due to Corona.

• GCE - Multi-D chemical space analysis: 
   
  UVES observations of seismic targets - p106  -> 47 hours + p105 -> 64 hours + TNG observations -> 7 hours.

  Additional 4.5 UVES hours for the observations used in the pilot project published in Valentini et al. 2019 + UVES for ~160 targets in two GCs -> 24 hours.