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I am an assistant astronomer working for the Centre de
Données (CDS) wich is
part of Strasbourg's observatory. My research interests are
linked to the formation and evolution of galaxies with a
particular emphasis on our host the Milky-Way.
My interests reside mainly (but not only) in understanding how
dynamical processes shape large disk galaxies such
as the Milky-Way or the Andromeda galaxy. To achieve my
goals, I use both numerical simulations (N-body and
hydrodynamical codes) and large surveys of stars in the
Galaxy that give access to the phase-space information
(position+velocities).
Below, you will find some more informations about the
projects I am currently involved in. This page is currently
under construction and more information will become available
as time permits.
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RAVE is an ambitious program to conduct a survey to
measure the radial velocities, metallicities and
abundance ratios for up to a million stars using the
1.2-m UK Schmidt Telescope of the Anglo-Australian
Observatory (AAO), over the period 2003-2010.
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The survey represents a giant leap forward in our understanding of
our own Milky Way galaxy, providing a vast stellar
kinematic database larger than any other survey proposed
for this coming decade. The main data product will be a
southern hemisphere survey of about a million
stars. This survey would comprise 0.7 million thin disk
main sequence stars, 250,000 thick disk stars, 100,000
bulge and halo stars, and a further 50,000 giant stars
including some out to 10 kpc from the Sun. RAVE will
offer the first truly representative inventory of
stellar radial velocities for all major components of
the Galaxy. Its completeness and homogeneity will make
it an invaluable stand-alone resource, but its full
potential will be realised when the radial velocities
are combined with proper motions and parallaxes from
other sources (USNO, Tycho).
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Gaia is a mission that will conduct a census of one thousand million stars in our Galaxy. It will monitor each of its target stars about 40 times over a five-year period, precisely charting their positions, distances, movements, and changes in brightness.
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