‘To contribute usefully to the scientific progress, one must sometimes not disdain from undertaking simple verifications’ (Foucault, 1847).
Despite the precautions taken when building the Gaia data processing, completely avoiding errors in a one billion+ source catalogue, with many intricate data for each object, is an impossible task. Before the publication of the Gaia archive, an in-depth validation of its contents has thus to be undertaken by the Gaia DPAC. It relies on methods and tools developed in the CU9 Work Package 940 in charge of the scientific validation of the catalogue.
Ensuring there are no systematic errors will lead to check for suspect spatial (or epoch, colour, magnitude, ...) variations, which could be due to observational or processing artefacts. The validation process will thus address the statistical distribution of the astrometric parameters, typically the unbiasedness of e.g. the parallaxes and proper motions, which are the main outcomes of the mission, and which may be subject to many perturbations. It will also scrutinize the photometric and spectroscopic data, assisted by the important classification task performed in Gaia, and, when available, external data.
Most of the validation work is being done with 8 work packages:
Besides the monthly telecons with the work package managers, it has been decided to have two plenary validation meetings per year.
This Paris meeting, which is the sixth plenary, will: