The ESO Large Programme First Stars
arXiv:0801.1293 · doi:10.1007/978-1-4020-9190-2_6
Abstract
In ESO period 65 (April-September 2000) the large programme 165.N-0276, led by Roger Cayrel, began making use of UVES at the Kueyen VLT telescope. Known within the Team and outside as ``First Stars'', it was aimed at obtaining high resolution, high signal-to-noise ratio spectra in the range 320 nm -- 1000 nm for a large sample of extremely metal-poor (EMP) stars identified from the HK objective prism survey.In this contribution we highlight the main results of the large programme.
to be published in the proceedings of the Workshop "Science with VLT in the ELT era" 8-12 October 2007, Garching, ed. A. Moorwood
References in corpus (4)
- First stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements
- First Stars VIII -- Enrichment of the neutron-capture elements in the early Galaxy
- First stars VII. Lithium in extremely metal poor dwarfs
- NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars