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Space Astrometry For Astrophysics
FUNDAMENTAL ASTRONOMY AND STELLAR SURVEYS
Conceptual Foundations of the Standard Celestial Reference System and Frame
Lecturer:
B. Bucciarelli
(INAF, Italy)
The Gaia mission
Lecturer:
J. de Bruijne
(ESA, The Netherlands)
An overview of current spectroscopic surveys
Lecturer:
S. BUDER
(MPIA)
ASTRONOMICAL METHODOLOGIES
From astrometry to distances and velocities, using Bayesian inference
Lecturer:
J. Rybizki
(MPIA, Germany)
Data driven approaches to deriving astrophysical parameters and ages
Lecturer:
A. Wheeler
(Columbia)
Reconstructing the selection function of your sample
Lecturer:
J. Rybizki
(MPIA, Germany)
GALACTIC DYNAMICS AND EVOLUTION OF THE MILKY WAY
Dynamical modelling techniques
Lecturer:
J. Hunt
(Toronto University, Canada)
Non-equilibrium signatures of the merging history of the Galaxy
Lecturer:
T. Antoja
(IEEC-UB, Spain)
Weighing the Galaxy with Gaia
Lecturer:
R. Sanderson
(University of Pennsylvania)
GLOBAL AND DIFFERENTIAL RELATIVISTIC ASTROMETRY
Some basics General Relativity for the beginner How to construct an astronomical reference system
Lecturer:
C. Le Poncin-Lafitte
(Obs. Paris, Syrte, France)
Global Astrometry in the Relativistic Context
Lecturer:
A. Vecchiato
(INAF, Italy)
Relativistic astrometric models in comparisons for Gaia
Lecturer:
S. Bertone
(GSFC/NASA, USA)
Differential Astrometry: Principles and Techniques
Lecturer:
B. Bucciarelli
(INAF, Italy)
Ray-tracing in Solar System How to solve the null geodesic equations
Lecturer:
C. Le Poncin-Lafitte
(Obs. Paris, Syrte, France)
CHEMO-KINEMATICS OF THE MILKY WAY
Galactic clusters resolved by Gaia
Lecturer:
J. de Bruijne
(ESA, The Netherlands)
The kinematics of the Galactic disc(s)
Lecturer:
T. Antoja
(IEEC-UB, Spain)
Unveiling the dynamical+chemical correlations in the Milky Way
Lecturer:
M. Ness
(Columbia University, USA)
The Galactic stellar halo
Lecturer:
R. Sanderson
(University of Pennsylvania)
SCIENCE AND PEOPLE
The richness of diversity in the new exploration of the Universe
Lecturer:
M. Branchesi
(Gran Sasso Science Institute, Italy)
The different spatio-temporal scales of the solar magnetism
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