activity
19942026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations · 64.6k across the 531 of their papers we have counts for

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Showing 2005Show all

13 papers · 1 filter

astro-ph2005★ 4 cited

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★ 429 cited

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-ph2005★ 40 cited

Enrichment of Very Metal-Poor Stars with Both r-Process and s-Process Elements from 8-10 M_\odot Stars

S. Wanajo, K. Nomoto, N. Iwamoto +2

Recent spectroscopic studies have revealed the presence of numerous carbon-enhanced, metal-poor stars with [Fe/H] < -2.0 that exhibit strong enhancements of s-process elements. The…

astro-ph2005★ 8 cited

The new record holder for the most iron-poor star: HE 1327-2326, a dwarf or subgiant with [Fe/H]=-5.4

A. Frebel, W. Aoki, N. Christlieb +16

We describe the discovery of HE 1327-2326, a dwarf or subgiant with [Fe/H]}=-5.4. The star was found in a sample of bright metal-poor stars selected from the Hamburg/ESO survey. It…

astro-ph2005★ 215 cited

HE1327-2326, an unevolved star with [Fe/H]<-5.0. I. A Comprehensive Abundance Analysis

W. Aoki, A. Frebel, N. Christlieb +17

We present the elemental abundances of HE1327-2326, the most iron-deficient star known, determined from a comprehensive analysis of spectra obtained with the Subaru Telescope High…

astro-ph2005★ 80 cited

The Origins of Two Classes of Carbon-Enhanced, Metal-Poor Stars

S. G. Ryan, W. Aoki, J. E. Norris +1

We have compiled composition, luminosity, and binarity information for carbon-enhanced, metal-poor (CEMP) stars reported by recent studies. We divided the CEMP star sample into two…

astro-ph2005★ 7 cited

The Metallicity Distribution Function of the Halo of the Milky Way

Timothy C. Beers, Norbert Christlieb, John E. Norris +8

We report on the distribution of metallicities, [Fe/H], for very metal-poor stars in the halo of the Galaxy. Although the primary information on the nature of the Metallicity Distr…

astro-ph2005★ 72 cited

Estimation of Carbon Abundances in Metal-Poor Stars. I. Application to the "Strong G-band" stars of Beers, Preston, & Shectman

Silvia Rossi, Timothy C. Beers, Chris Sneden +3

We develop and test a method for the estimation of metallicities ([Fe/H]) and carbon abundance ratios ([C/Fe]) for carbon-enhanced metal-poor (CEMP) stars, based on application of…

astro-ph2005★ 24 cited

The Century Survey Galactic Halo Project II: Global Properties and the Luminosity Function of Field Blue Horizontal Branch Stars

Warren R. Brown, Margaret J. Geller, Scott J. Kenyon +4

We discuss a 175 deg^2 spectroscopic survey for blue horizontal branch (BHB) stars in the Galactic halo. We use the Two Micron All Sky Survey (2MASS) and the Sloan Digital Sky Surv…

astro-ph2005★ 504 cited

The Hamburg/ESO R-process Enhanced Star survey (HERES) II. Spectroscopic analysis of the survey sample

P. S. Barklem, N. Christlieb, T. C. Beers +7

We present the results of analysis of ``snapshot'' spectra of 253 metal-poor halo stars -3.8 < [Fe/H] < -1.5 obtained in the HERES survey. The spectra are analysed using an automat…

astro-ph2005★ 566 cited

Nucleosynthetic signatures of the first stars

Anna Frebel, Wako Aoki, Norbert Christlieb +16

The chemically most primitive stars provide constraints on the nature of the first stellar objects that formed in the Universe; elements other than hydrogen, helium and traces of l…

astro-ph2005★ 15 cited

Kinematics of the Galactic Halo from Horizontal Branch stars in the Hamburg/ESO Survey

Christopher Thom, Chris Flynn, Michael S. Bessell +6

Large samples of Field Horizontal Branch (FHB) stars make excellent tracers of the Galactic halo; by studying their kinematics, one can infer important physical properties of our G…

astro-ph2005★ 198 cited

Spectroscopic Studies of Very Metal-Poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements

Wako Aoki, Satoshi Honda, Timothy C. Beers +7

Elemental abundance measurements have been obtained for a sample of 18 very metal-poor stars using spectra obtained with the Subaru Telescope High Dispersion Spectrograph. Seventee…