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V. Zh. Adibekyan

Researcher at University of Porto

Publications -  27
Citations -  2988

V. Zh. Adibekyan is an academic researcher from University of Porto. The author has contributed to research in topics: Stars & Metallicity. The author has an hindex of 22, co-authored 27 publications receiving 2788 citations.

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Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program - Galactic stellar populations and planets

TL;DR: In this article, a uniform and detailed analysis of 12 refractory elements (Na, Mg, Al, Si, Ca, Ti, Cr, Ni, Co, Sc, Mn, and V) was performed for a sample of 1111 FGK dwarf stars from the HARPS GTO planet search program.
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Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

Rodolfo Smiljanic, +101 more
TL;DR: In this paper, the Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT, which are analyzed in parallel by several state-of-the-art methodologies.
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The Gaia-ESO Survey: the analysis of high-resolution UVES spectra of FGK-type stars

Rodolfo Smiljanic, +110 more
TL;DR: In this article, the Gaia-ESO Public Spectroscopic Survey is using FLAMES at the VLT to obtain high-quality medium-resolution Giraffe spectra for about 10(5) stars and high-resolution UVES spectra of about 5000 stars.
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A new α-enhanced super-solar metallicity population

TL;DR: In this article, a uniform and detailed analysis of 1112 high-resolution spectra of FGK-dwarfs obtained with the HARPS spectrograph at the ESO 3.6m telescope was performed.
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Deriving precise parameters for cool solar-type stars Optimizing the iron line list ?;??;???

TL;DR: In this paper, the authors compare the differences in temperature between the standard spectroscopic technique based on iron lines and the infrared flux method (IRFM) and show that the differences for the cooler stars are significantly smaller and more homogeneously distributed than in previous studies.