4.6 Article

Gaia Early Data Release 3: Catalogue validation

Journal

ASTRONOMY & ASTROPHYSICS
Volume 649, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/202039834

Keywords

catalogs; astrometry; techniques: photometric

Funding

  1. Spanish Ministry of Science, Innovation and University (MICIU/FEDER, UE) [RTI2018-095076-B-C21, ESP2016-80079C2-1-R]
  2. Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia 'Maria de Maeztu') [MDM-2014-0369, CEX2019-000918-M]
  3. Agenzia Spaziale Italiana (ASI) [2014-025R.0, 2014-025-R.1.2015, 2018-24-HH.0]
  4. European Research Council (ERC) under the European Union [695099]
  5. French Agence Nationale de la Recherche (ANR) [ANR-15-CE31-0012-01]

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The third Gaia data release, consisting of Gaia EDR3 and Gaia DR3, provides precise astrometric and photometric properties for nearly two billion sources, along with radial velocities from Gaia DR2. The validation processes ensure completeness, accuracy, and precision of the data, offering recommendations for dealing with various issues related to the catalog data.
Context. The third Gaia data release is published in two stages. The early part, Gaia EDR3, gives very precise astrometric and photometric properties for nearly two billion sources together with seven million radial velocities from Gaia DR2. The full release, Gaia DR3, will add radial velocities, spectra, light curves, and astrophysical parameters for a large subset of the sources, as well as orbits for solar system objects. Aims. Before the publication of the catalogue, many different data items have undergone dedicated validation processes. The goal of this paper is to describe the validation results in terms of completeness, accuracy, and precision for the Gaia EDR3 data and to provide recommendations for the use of the catalogue data. Methods. The validation processes include a systematic analysis of the catalogue contents to detect anomalies, either individual errors or statistical properties, using statistical analysis and comparisons to the previous release as well as to external data and to models. Results.Gaia EDR3 represents a major step forward, compared to Gaia DR2, in terms of precision, accuracy, and completeness for both astrometry and photometry. We provide recommendations for dealing with issues related to the parallax zero point, negative parallaxes, photometry for faint sources, and the quality indicators.

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