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19992023
most citedFirst stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

1.2k citations · 16.7k across the 138 of their papers we have counts for

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astro-ph2008★ 145 cited

NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars

S. M. Andrievsky, M. Spite, S. A. Korotin +5

Aims: Aluminium is a key element to constrain the models of the chemical enrichment and the yields of the first supernovae. But obtaining precise Al abundances in extremely metal-p…

astro-ph2008★ 332 cited

The kinematic status and mass content of the Sculptor dwarf spheroidal galaxy

G. Battaglia, A. Helmi, E. Tolstoy +3

We present VLT/FLAMES spectroscopic observations (R~6500) in the CaII triplet region for 470 probable kinematic members of the Sculptor (Scl) dwarf spheroidal galaxy. The accurate…

astro-ph2008★ 2 cited

The ESO Large Programme First Stars

P. Bonifacio, J. Andersen, S. Andrievsky +19

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…

astro-ph2007★ 55 cited

First Stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876--032

J. I. González Hernández, P. Bonifacio, H. -G. Ludwig +15

We have used high-resolution, high-S/N ratio spectra from the UVES spectrograph at the ESO VLT telescope. Long-term radial-velocity measurements and broad-band photometry allow us…

astro-ph2007★ 211 cited

Analysis and calibration of CaII triplet spectroscopy of Red Giant Branch stars from VLT/FLAMES observations

G. Battaglia, M. Irwin, E. Tolstoy +4

We demonstrate that low resolution CaII triplet (CaT) spectroscopic estimates of the overall metallicity ([Fe/H]) of individual Red Giant Branch (RGB) stars in two nearby dwarf sph…

astro-ph2006★ 226 cited

First stars VII. Lithium in extremely metal poor dwarfs

P. Bonifacio, P. Molaro, T. Sivarani +12

Aims. This study aims to determine the level and constancy of the Spite plateau as definitively as possible from homogeneous high-quality VLT-UVES spectra of 19 of the most metal-p…