DPAC Executive membership (DPACE): Leading the Gaia Data Reduction and Analysis Consortium, DPAC. Michael Biermann is a DPACE member since 2016. DPAC is the Gaia Data Processing and Analysis Consortium, ESA's official science partner in the Gaia project. Ulrich Bastian was DPAC member from 2004 to 2016.
DPAC Project Office: Supporting the DPAC Executive, controlling the consortium, scheduling its activities. The DPAC Project Office is located at ESAC (Villafranca, Spain). It is staffed from several countries contributing to Gaia/DPAC. Its leader Gonzalo Garcia (since 2015) from ARI. The ARI members Emmanuel Mercier and Sebastian Els filled this position between 2008-2013 and 2013-2015, respectively.
Gaia Science Team membership: Consulting ESA on all scientific aspects of Gaia (Ulrich Bastian 2002-2007, Eva Grebel 2007-2009). The Gaia Science Team is composed of independent scientists with specific scientific and/or technical expertise relevant to Gaia.
CU3 Leadership: Leading and managing Coordination Unit 3, "Core Processing", one of DPAC's nine subdivisions (Michael Biermann, since 2015, Ulrich Bastian, from 2006 to 2015). CU3 has more than 100 members, mostly astronomers and software engineers, scattered all over Europe, plus a small group in Brasil. The task of CU3 is to organise and implement the data processing chain all the way from receiving Gaia's raw telemetry down to the core astrometric solution.
First Look Leadership: Quickly assessing payload and data health, and scientific data quality (Manager Wolfgang Löffler, Marcus Hauser 2015-2018, Michael Biermann 2011-2015, Stefan Jordan 2006-2011). First Look (FL) is one of the major building blocks of CU3. Most of the work for this task is done at ARI, but software modules from many other DPAC groups have to be included into the overall system which comprised 350 000 lines of java program code at the end of 2011.
Eduardo Peloso (software developer) and Zoltán Balog (first-look scientist) have joint the first-look team in 2018.
Important former contributions to First Look: Ulrike Stampa , Thomas Brüsemeister, Stefan Jordan, Ulrich Bastian
Ecliptic-poles catalogue: At the beginning of the Gaia mission Preparing an special scanning law was used for the initial calibration and verification of the Gaia spacecraft and operations (Martin Altmann, Ulrich Bastian) in which the ecliptic poles were observable by Gaia at each rotation. Two carefully prepared sky inventories of the order of a square degree were created for this purpose.
Ground-based optical tracking: Organising a 5-year observing campaign to reach the tremendous orbit determination precision needed for Gaia (Martin Altmann, Ulrich Bastian). Gaia's astrometry reduction needs to know the velocity of the spacecraft with respect to the solar-system barycentre to a precision of 2.5 mm/s at all times. An orbit determination to this precision is almost impossible to reach with the usual tracking methods. But using daily astrometric observations of the Gaia spacecraft from the ground will do the job.
Mixed core processing contributions: Providing conventions and interface softwares to DPAC (Helmut Lenhardt, Ulrich Bastian). Topics covered include softwares for barycentric velocity corrections, for light-travel time corrections, for local coordinates on the sky etc., as well as precise definitions of reference systems and datation schemes to be used throughout the consortium, and the setting of conventional values of Nature's constants.
Public Outreach (Leadership): Leading and managing the workpackage for Public Outreach and Education for DPAC (Stefan Jordan). Providing brochures, posters, public talks, introductory presentations, internet articles, 3D dome animations, German info materials etc.. (Toni Sagristà Sellés, Ulrich Bastian, and Markus Pössel from the Haus der Astronomie).
Gaia Database at ARI: Delivering, documenting and presenting the Gaia scientific results to the community (Stefan Jordan, Markus Demleitner, Grégory Mantelet, Jon Juaristi).
Contributions to Gaia Working Groups
ESA/DPAC Gaia Calibration and Operations Working Group: Michael Biermann