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20022026
most citedThe Chandra COSMOS Survey, I: Overview and Point Source Catalog

445 citations · 5.8k across the 102 of their papers we have counts for

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Showing 2014 · astro-ph.SRShow all

7 papers · 2 filters

astro-ph.SR2014★ 73 cited

The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge

L. Howes, M. Asplund, A. R. Casey +39

We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars s…

astro-ph.SR2014★ 227 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.SR2014

The Chandra Cygnus OB2 Legacy Survey: Design and X-ray Point Source Catalog

Nicholas J. Wright, Jeremy J. Drake, Mario G. Guarcello +5

The Cygnus OB2 association is the largest concentration of young and massive stars within 2 kpc of the Sun, including an estimated 65 O-type stars and hundreds of OB stars. The Cha…

astro-ph.SR2014★ 80 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…

astro-ph.SR2014★ 42 cited

The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region

L. Spina, S. Randich, F. Palla +37

Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun…

astro-ph.SR2014★ 36 cited

The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster Gamma Velorum

L. Spina, S. Randich, F. Palla +36

Knowledge of the abundance distribution of star forming regions and young clusters is critical to investigate a variety of issues, from triggered star formation and chemical enrich…

astro-ph.SR2014★ 133 cited

The Gaia-ESO Survey: Kinematic structure in the Gamma Velorum Cluster

R. D. Jeffries, R. J. Jackson, M. Cottaar +27

Context: A key science goal of the Gaia-ESO survey (GES) is to use the kinematics of low-mass stars in young clusters to probe their dynamical histories and how they populate the f…