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# System prepended metadata

title: INT run -- after Gaia DR3

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# 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)
