ARI contributions to Gaia
Contributions to Gaia management
DPAC Executive membership:
Leading the Gaia Data Reduction and Analysis Consortium, DPAC (Ulrich Bastian, since 2004). DPAC is the Gaia Data Processing and Analysis Consortium, ESA's official science partner in the Gaia project.
DPAC Project Office:
Supporting the DPAC Executive, controlling the consortium (Emmanuel Mercier, since 2008), 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 is from ARI.
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.
Leading and managing Coordination Unit 3, "Core Processing", one of DPAC's eight subdivisions (Ulrich Bastian, since 2006). CU3 has 102 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 (Michael Biermann, deputy Marcus Hauser). 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 Biermann, Ulrike Stampa , Thomas Brüsemeister), in collaboration with the Gaia Science Operations Centre at ESAC Villafranca, Spain.
One-Day Astrometric Solution,
Calibrating Gaia quickly and continuously (Michael Biermann, Wolfgang Löffler, Stefan Jordan, Ulrich 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 being implemented.
FL Monitor and FL Evaluator:
Diagnosing and assessing the health and quality of the Gaia data (Michael Biermann, Marcus Hauser, Wolfgang Löffler, Shilpa Aguduri, Thomas Brüsemeister, Ulrike Stampa). The FL Monitor software compiles a vast variety of statistics and diagnostics, both from the pre-processed raw data of Gaia and from the results of the ODAS and 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.
Executing the First Look (Michael Biermann, Marcus Hauser). 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 as well as industry-derived design and laboratory data, and 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)
Preparing an important tool for the initial calibration and verification of the Gaia spacecraft and operations (Martin Altmann, Ulrich 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 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.
Providing public talks, introductory presentations at astronomical institutes, Wikipedia articles, German info materials etc. (Ulrich Bastian, Stefan Jordan, Wilfried Hofmann)
Gaia Results Database:
Delivering, documenting, presenting the Gaia scientific results to the community (Stefan Jordan, Shilpa Aguduri). This topic will be treated by a specific DPAC coordination unit, CU9, to be created in 2012 after a dedicated announcement of opportunity expected from ESA. The true task will be to make the Gaia results as easily understandable, as comfortably accessible and as widely usable as possible. The precise distribution of work packages for CU9 is being discussed in the Euroope-wide Gaia Access Preparation group (GAP).
Contributions to Gaia Working Groups
ESA/DPAC Gaia Calibration and Operations Working Group:
DPAC Radiation task force:
DPAC Operations Steering Group
Ground-based Observations Group: