A. de Torres

TL;DR: In this article, the authors used the Gaia Early Data Release 3 (EDR3) for the study of the Milky Way structure and evolution, including the disturbances of the current disc, the spatial and kinematical distributions of early accreted versus in-situ stars, the structures in the outer parts of the disc, and the orbits of open clusters Berkeley 29 and Saurer 1.

TL;DR: An error occurred during the production process of the original published version as mentioned in this paper and the following names were omitted from the author list: R. Haigron, D. Hatzidimitriou, M. Hauser, E. Haywood, U. Heiter, J. Heu, T. Hilger.

TL;DR: Gaia DR3 as discussed by the authors provides a powerful and precise view of the Milky Way with unprecedented spatial coverage and statistical robustness, revealing the strong vertical symmetry of the Galaxy and the flared structure of the disc.

TL;DR: The Gaia DR3 Catalogue as mentioned in this paper contains about eight hundred thousand solutions with either orbital elements or trend parameters for astrometric, spectroscopic and eclipsing binaries, and combinations of them.

TL;DR: In this article , the authors select various stellar populations to explore and identify non-axisymmetric features in the disc of the Milky Way in both configuration and velocity space using the Gaia DR3 data.