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Gaia Satellite > ARI contributions to Gaia

ARI contributions to Gaia

Contributions to Gaia management

  • 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.

DPAC Workpackages

  • 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 Marcus Hauser since 2015, 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. The following four FL functions are specifically located at ARI.

    • First-Look processing framework: 
      Developing the software needed to run the various FL processes (Wolfgang Löffler, Michael BiermannUlrike Stampa Thomas Brüsemeister), in collaboration with the Gaia Science Operations Centre at ESAC Villafranca, Spain.
    • One-Day Astrometric Solution, ODAS: 
      Calibrating Gaia quickly and continuously (Marcus Hauser, Michael BiermannWolfgang Löffler,  Stefan JordanUlrich Bastian, ). A high-precision astrometric calibration of both the instrument and the observed sky is needed to make an exploration into the data quality at microarcsec level possible. A method to do this on a daily basis is implemented.
    • FL Monitor and FL Evaluator: 
      Diagnosing and assessing the health and quality of the Gaia data (Michael BiermannMarcus HauserWolfgang Löffler, Thomas Brüsemeister, Ulrike Stampa, Ulrich Bastian, Stefan Jordan). The FL Monitor software compiles a vast variety of statistics and diagnostics, both from the pre-processed raw data of Gaia, from the results of the ODAS and from several other so-called one-day calibrations. The FL Evaluator software aids the FL Scientist to inspect and judge the vast Monitor outputs, in order to verify the proper working of the spacecraft and instruments.
    • First-Look Scientist(s): 
      Executing the First Look ( Marcus Hauser, Michael Bierman). The First-Look Scientist in charge will be the human part of the FL Evaluator. He will do the daily assessment of the FL results and decide whether operational consequences should be proposed to the Mission Operations Centre and/or whether special quick investigations into the data be proposed to other DPAC groups.

  • Auxiliary data management: 
    Coordinating the acquisition of input data for CU3 that are not produced by Gaia itself (Ulrich Bastian). The astrometric reduction of the Gaia observations needs a broad variety of external input data, including e.g. ground-based astronomical observations of reference and calibration stars, industry-derived design and laboratory data, as all as orbit determination results from ESOC. The following three sets of data are specifically taken care of by ARI.

    • Initial calibration data: 
      Planning and surveying the influx of laboratory data from industry and ESA before launch, and of early in-flight calibrations from the commissioning phase after launch (Marcus Hauser)
    • Ecliptic-poles catalogue: 
      Preparing an important tool for the initial calibration and verification of the Gaia spacecraft and operations (Martin AltmannUlrich Bastian). The ecliptic poles are the only sky areas observable by Gaia at any time. Two carefully prepared sky inventories of the order of a square degree will be used both in the commissioning phase after launch and in cases of contingency.

  • Ground-based optical tracking: 
    Organising a 5-year observing campaign to reach the tremendous orbit determination precision needed for Gaia (Martin AltmannUlrich 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 LenhardtUlrich 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 SellésUlrich Bastian, and  Markus Pössel from the Haus der Astronomie).
  • Gaia Results Database: 
    Delivering, documenting and presenting the Gaia scientific results to the community (Stefan JordanMarkus Demleitner, Grégory Mantelet). The task will be to make the Gaia results as easily understandable, as comfortably accessible and as widely usable as possible.

Contributions to Gaia Working Groups

  • ESA/DPAC Gaia Calibration and Operations Working Group: 
    Michael Biermann

  • GaiaTools Committee: 
    Wolfgang Löffler

  • DPAC Radiation task force: 
    Stefan Jordan

  • DPAC Operations Steering Group 
    Ulrich Bastian

  • Ground-based Observations Group: 
    Martin Altmann
Editor: Stefan Jordan
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