activity
19942023
most citedThe MACHO Project: Microlensing Results from 5.7 Years of LMC Observations

1k citations · 22.8k across the 263 of their papers we have counts for

collaborators
Showing 2011 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2011

First Results for the Solar Neighborhood of the Asiago Red Clump Survey

M. Valentini, U. Munari, T. Saguner +4

The Asiago Red Clump Spectroscopic Survey (ARCS) is an ongoing survey that provides atmospheric parameters, distances and space velocities of a well selected sample of Red Clump st…

astro-ph.GA2011★ 79 cited

The RAVE catalogue of stellar elemental abundances: first data release

C. Boeche, A. Siebert, M. Williams +21

We present chemical elemental abundances for stars observed by the RAdial Velocity Experiment (RAVE), an ambitious spectroscopic survey of our Galaxy at Galactic latitudes…

astro-ph.GA2011★ 57 cited

Distance determination for RAVE stars using stellar models III: The nature of the RAVE survey and Milky Way chemistry

B. Burnett, J. Binney, S. Sharma +19

We apply the method of Burnett & Binney (2010) for the determination of stellar distances and parameters to the internal catalogue of the Radial Velocity Experiment (Steinmetz et a…

astro-ph.GA2011★ 172 cited

The RAdial Velocity Experiment (RAVE): Third Data Release

A. Siebert, M. E. K. Williams, A. Siviero +36

We present the third data release of the RAdial Velocity Experiment (RAVE) which is the first milestone of the RAVE project, releasing the full pilot survey. The catalog contains 8…

astro-ph.GA2011★ 177 cited

The Case for the Dual Halo of the Milky Way

Timothy C. Beers, Daniela Carollo, Zeljko Ivezic +11

Carollo et al. have recently resolved the stellar population of the Milky Way halo into at least two distinct components, an inner halo and an outer halo. This result has been crit…

astro-ph.GA2011★ 141 cited

Carbon-Enhanced Metal-Poor Stars in the Inner and Outer Halo Components of the Milky Way

D. Carollo, T. C. Beers, J. Bovy +6

(Abridged) Carbon-enhanced metal-poor (CEMP) stars in the halo components of the Milky Way are explored, based on accurate determinations of the carbon-to-iron ([C/Fe]) abundance r…