most citedThe SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open Clusters

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astro-ph2007316 cited

The SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open Clusters

Y. S. Lee, T. C. Beers, T. Sivarani +13

We validate the performance and accuracy of the current SEGUE (Sloan Extension for Galactic Understanding and Exploration) Stellar Parameter Pipeline (SSPP), which determines stell…

astro-ph2007511 cited

The SEGUE Stellar Parameter Pipeline. I. Description and Initial Validation Tests

Y. S. Lee, T. C. Beers, T. Sivarani +10

We describe the development and implementation of the SEGUE (Sloan Extension for Galactic Exploration and Understanding) Stellar Parameter Pipeline (SSPP). The SSPP derives, using…

astro-ph2005

SDSSJ103913.70+533029.7: A Super Star Cluster in the Outskirts of a Galaxy Merger

G. R. Knapp, C. A. Tremonti, C. M. Rockosi

We describe the serendipitous discovery in the spectroscopic data of the Sloan Digital Sky Survey of a star-like object, SDSSJ103913.70+533029.7, at a heliocentric radial velocity…

astro-ph2005

A Spectroscopic Study of the Ancient Milky Way: F- and G-Type Stars in the Third Data Release of the Sloan Digital Sky Survey

C. Allende Prieto, T. C. Beers, R. Wilhelm +4

(Abridged) We perform an analysis of spectra and photometry for 22,770 stars included in the third data release (DR3) of the SDSS. We measure radial velocities and, based on a mode…

astro-ph2004

High-Resolution Spectroscopy of the Transiting Planet Host Star TrES-1

A. Sozzetti, D. Yong, G. Torres +6

We report on a spectroscopic determination of the stellar parameters and chemical abundances for the parent star of the transiting planet TrES-1. Based on a detailed analysis of ir…

astro-ph2003

Magnesium isotope ratios in Hyades stars

David Yong, David L. Lambert, Carlos Allende Prieto +1

Using classical model atmospheres and an LTE analysis, Mg isotope ratios 24Mg:25Mg:26Mg are measured in 32 Hyades dwarfs covering 4000K < Teff < 5000K. We find no significant trend…