activity
19952026
most citedAn absolutely calibrated effective temperature scale from the InfraRed Flux Method

724 citations · 11.7k across the 132 of their papers we have counts for

collaborators
Showing 2006Show all

6 papers · 1 filter

astro-ph2006★ 79 cited

Chemical Abundance Analysis of the Extremely Metal-Poor Star HE 1300+0157

Anna Frebel, John E. Norris, Wako Aoki +5

We present a detailed chemical abundance analysis of HE 1300+0157, a subgiant with [Fe/H]=-3.9. From a high-resolution, high-S/N Subaru/HDS spectrum we find the star to be enriched…

astro-ph2006★ 138 cited

Chemical Homogeneity in Collinder 261 and Implications for Chemical Tagging

G. M. De Silva, K. C. Freeman, M. Asplund +3

This paper presents abundances for 12 red giants of the old open cluster Collinder 261 based on spectra from VLT/UVES. Abundances were derived for Na, Mg, Si, Ca, Mn, Fe, Ni, Zr an…

astro-ph2006★ 125 cited

Chemically Tagging the HR1614 Moving Group

G. M. De Silva, K. C. Freeman, J. Bland-Hawthorn +2

We present abundances for a sample of F,G,K dwarfs of the HR1614 moving group based on high resolution, high S/N ratio spectra from AAT/UCLES. Our sample includes stars from Feltzi…

astro-ph2006★ 113 cited

The Carina-Near Moving Group

B. Zuckerman, M. S. Bessell, Inseok Song +1

We identify a group of ~20 co-moving, mostly southern hemisphere, ~200 Myr old stars near Earth. Of the stars likely to be members of this Carina-Near Moving Group, in either its n…

astro-ph2006★ 194 cited

Bright Metal-Poor Stars from the Hamburg/ESO Survey. I. Selection and Follow-up Observations from 329 Fields

A. Frebel, N. Christlieb, J. E. Norris +9

We present a sample of 1777 bright (9<B<14) metal-poor candidates selected from the Hamburg/ESO Survey (HES). Despite saturation effects present in the red portion of the HES objec…

astro-ph2006★ 43 cited

A deep photometric survey of the eta Chamaeleontis cluster down to the brown dwarf - planet boundary

A-Ran Lyo, Inseok Song, Warrick A. Lawson +2

We report the outcome of the deep optical/infrared photometric survey of the central region (33 X 33 arcmin or 0.9 pc^2) of the eta Chamaeleontis pre-main sequence star cluster. Th…