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Damian Fabbian

Researcher at Spanish National Research Council

Publications -  43
Citations -  3767

Damian Fabbian is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Stars & Spectral line. The author has an hindex of 17, co-authored 42 publications receiving 3613 citations. Previous affiliations of Damian Fabbian include Australian National University & Max Planck Society.

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The tenth data release of the Sloan digital sky survey: First spectroscopic data from the SDSS-iii apache point observatory galactic evolution experiment

Christopher P. Ahn, +275 more
TL;DR: The 10th public data release (DR10) from the Sloan Digital Sky Survey (SDSS-III) was released in 2013 as mentioned in this paper, which includes the first spectroscopic data from the Apache Point Observatory Galaxy Evolution Experiment (APOGEE), along with spectroscopy data from Baryon Oscillation Spectroscopic Survey (BOSS) taken through 2012 July.
Journal ArticleDOI

The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment

Christopher P. Ahn, +234 more
TL;DR: SDSS-III as discussed by the authors contains the first spectroscopic data from the Apache Point Observatory Galaxy Evolution Experiment (APOGEE), along with spectra from the Baryon Oscillation Spectroscopic Survey (BOSS) taken through 2012 July.
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Target selection for the apache point observatory galactic evolution experiment (apogee)

TL;DR: The Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution infrared spectroscopic survey spanning all Galactic environments (i.e., bulge, disk, and halo), with the principal goal of constraining dynamical and chemical evolution models of the Milky Way as discussed by the authors.
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Sulphur and zinc abundances in Galactic halo stars revisited

TL;DR: In this article, a new set of sulphur abundances in very metal-poor stars and an improved analysis of previous data were derived from the VLT/UVES spectra of 40 main-sequence stars with −3.3 < [Fe/H] < −1.0.
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The C/O ratio at low metallicity: constraints on early chemical evolution from observations of Galactic halo stars

TL;DR: In this paper, the abundances of carbon and oxygen derived from high-excitation C i and O i absorption lines in metal-poor halo stars were analyzed, with an emphasis on additional C/O determinations in the crucial metallicity range −3 < [Fe/H] < −2.