A research project in collaboration between the SAGA Team at CAMK/PAN
and the group of Prof. Norbert Christlieb (University of Heidelberg)
"The old Milky Way: a holistic approach for the accurate analysis of metal-poor stars"
Funded by an OPUS + LAP/ Weave grant from NCN (2022/47/I/ST9/02358) and DFG
Characterise with high accuracy all known very metal-poor stars
The S2 high-resolution halo survey organized a hackaton in Heidelberg, Germany, for the analysis of the first batch of 4MOST data.
The paper "Estimating stellar metallicities from Gaia DR3 XP data using LAMOST DR10" has been accepted for publication in Astronomy & Astrophysics.
HRMOS is a very high spectral resolution (80k) multi-object (50-60) spectrograph that will be proposed as a next generation instrument for the VLT. The white paper presents the scientific rationale HRMOS and the instrument concept.