# INT run -- after Gaia DR3

:pencil: Anke Arentsen (A), Nicolas Martin (M), Rodrigo Ibata (I), Zhen Yuan (Y)

## :calendar: Schedule
- June (5 nights, starts from Friday)
- July

## :book: Shared Files

## :Pencil: Plan

- HVS
- searching high pm, no rv in DR3 RVS
- prepare the table from EDR3. magnitude G_RVS <= 16 (?), high pm (>25 mas/yr for stars without distance), vt>600 km/s (stars with distance) [name=A]
- MS has good distance, most of Giants closer than 15 kpc

- PristineEMP

- EMP Spec sample x RVS
- Pristine I

- bright Pristine LM that has no metallicity info in RVS
- check the limit of RVS metallicity (RAVE, Galah) [name=Y]
- follow bright PristineEMP Giants
- training sample (SDSS [Fe/H]_adop, LAMOST DR8)

- SF [name=I]
- SFxPristine: more Pristine coverage
- New low-metallicity streams followup
- SFxAllSky(Pristine-like)
- [Fe/H]pris vs. [Fe/H]BP/RP [name=M]

- CEMP
- [name=A] shares HR sample [name=Y]
- decide the next followup (week after EAS)