activity
19972005
most citedThe GAIA Astrometric Survey of the Solar Neighborhood and its Contribution to the Target Database for DARWIN/TPF

3 citations · 3 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph2005

Structure in the motions of the fastest halo stars

P. ReFiorentin, A. Helmi, M. G. Lattanzi +1

We have analyzed the catalog of 2106 non-kinematically selected metal poor stars in the solar neighborhood published by Beers et al. (2000), with the goal of quantifying the amount…

astro-ph20033 cited

The GAIA Astrometric Survey of the Solar Neighborhood and its Contribution to the Target Database for DARWIN/TPF

A. Sozzetti, S. Casertano, M. G. Lattanzi +1

We evaluate the potential of the ESA Cornerstone Mission GAIA in helping populate the database of nearby stars ( pc) for subsequent target selection for DARWIN/TPF. The GAI…

astro-ph2002

Galaxy structure and kinematics towards the NGP

A. Spagna, C. Cacciari, R. Drimmel +3

We present a proper motion survey over about 200 square degrees towards the NGP, based on the material used for the construction of the GSC-II, that we are using to study the verti…

astro-ph2002

Faint and peculiar objects in GAIA: results from GSC-II

D. Carollo, A. Spagna, M. G. Lattanzi +3

The one billion objects in the GSC-II make up a formidable data set for the hunt of peculiar and rare targets such as late type stars, white dwarfs, carbon dwarfs, asteroids, varia…

astro-ph1997

Hipparcos Positioning of Geminga : How and Why

P. A. Caraveo, M. G. Lattanzi, G. Massone +4

Accuracy in the absolute position in the sky is one of the limiting factors for pulsar timing, and timing parameters have a direct impact on the understanding of the physics of Iso…

astro-ph1997

Distances and Absolute Ages of Galactic Globular Clusters from Hipparcos Parallaxes of Local Subdwarfs

R. G. Gratton, F. Fusi Pecci, E. Carretta +3

High precision trigonometric parallaxes from the HIPPARCOS satellite and accurate metal abundances ([Fe/H], [O/Fe], and [alpha/Fe]) from high resolution spectroscopy for about 30 l…