Objectif
The coordination unit CU6 is part of the Gaia
Data Processing and Analysis Consortium (DPAC). Within this frame, it will be
in charge of the ground-based processing and analysis of the Gaia spectroscopic
data, i.e. the data obtained with Radial Velocity Spectrometer
(RVS). Its goal is to derive radial velocities and rotation velocities
for all the stars observed with the RVS (up to magnitude 16-17), and atmospheric
parameters and element abundances for the brightest part of the programme. In
addition, the Radial Velocity Spectrometer multi-epoch observations are well
suited for the identification, classification and characterisation of the many
types of double, multiple and variable stars.
For any question related to Coordination unit CU6, please contact
David KATZ, GEPI,
Observatoire de Paris, Section de Meudon
For any question related to CU6 web site or documentation, please contact
Catherine Turon,GEPI,
Observatoire de Paris, Section de Meudon
Group members
Workshops
and meetings
Work breakdown
and CU6 structure
RVS charateristics
Actions
Development
Cycle 2
Bibliography