activity
20142023
most citedGaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

227 citations · 422 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20233 cited

Metal-poor stars observed with the Magellan Telescope. IV. Neutron-capture element signatures in 27 main-sequence stars

Mohammad K. Mardini, Anna Frebel, Leyatt Betre +3

Based on high-resolution spectra obtained with Magellan/MIKE, we present a chemo-dynamical analysis for 27 near main-sequence turnoff metal-poor stars, including 20 stars analyzed…

astro-ph.SR201631 cited

The Gaia-ESO Survey: the inner disk, intermediate-age open cluster Trumpler 23

J. C. Overbeek, E. D. Friel, P. Donati +33

Context: Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a Rgc ~6 kpc. It is in a crowded field very close to the Galactic plane and…

astro-ph.SR201430 cited

The Chemical Evolution of Phosphorus

Heather R. Jacobson, Thanawuth Thanathibodee, Anna Frebel +3

Phosphorus is one of the few remaining light elements for which little is known about its nucleosynthetic origin and chemical evolution, given the lack of optical absorption lines…

astro-ph.SR201451 cited

Detection of Neutral Phosphorus in the Near Ultraviolet Spectra of Late-Type Stars

Ian U. Roederer, Heather R. Jacobson, Thanawuth Thanathibodee +2

We report the detection of several absorption lines of neutral phosphorus (P, Z=15) in archival near ultraviolet spectra obtained with the Space Telescope Imaging Spectrograph on b…

astro-ph.SR2014227 cited

Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

R. Smiljanic, A. J. Korn, M. Bergemann +99

The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-t…

astro-ph.SR201480 cited

The Gaia-ESO Survey: Stellar content and elemental abundances in the massive cluster NGC 6705

T. Cantat-Gaudin, A. Vallenari, S. Zaggia +52

Chemically inhomogeneous populations are observed in most globular clusters, but not in open clusters. Cluster mass seems to play a key role in the existence of multiple population…