Gaia Mission

The First Look of Gaia: Daily Data Quality And Instrument Health Assessment With Automated Early Warnings

By Keith Cowing
Status Report
astro-ph.IM
May 7, 2026
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The First Look of Gaia: Daily Data Quality And Instrument Health Assessment With Automated Early Warnings
Sky coverage (given in equatorial coordinates) of two FL days spaced about one month apart. The blue pattern is the complete Gaia sky coverage starting at OBMT=10,000 rev to the end of operations (OBMT=16,385.671 rev), the red track represents a FL day that lasted from January 4 to 5, 2023, and the orange track another day, between February 4 and 5, 2023. In this plot the trace for just the first telescope (FoV 1) is shown. — astro-ph.IM

Editor’s note: according to NASA: “With its all-sky survey of the position, brightness and motion of over one billion stars in our Milky Way galaxy, Gaia will provide a large dataset to search for exoplanets. These will be uncovered by monitoring tiny changes in a star’s position and motion caused by the gravitational pull of one or more planets around it, and by looking for dips in the stellar light caused by a planet transiting in front of its parent star.”


The ESA Gaia mission is a 10+ year astrometric whole-sky scan, demanding consistent data quality over the whole timespan of operations

Aims. The Gaia First Look (FL) is a system whose aim is monitoring the data quality to identify problems, which includes early warning capabilities for potential upcoming issues.

Methods. In order to achieve its goals, the Gaia FL implemented its own limited astrometric solution, and used the daily calibrations from other segments of the Data Processing and Analysis Consortium (DPAC), as well as the diagnostic data from the satellite itself, in order to obtain a complete picture of the situation of the Gaia satellite on a daily basis.

This led to a short-term health and data quality check, but also to a broader overview of the longer-term trends and evolutions within the payload. Potential issues that were encountered were reported to other groups within DPAC for further analysis purposes. When required, ways to mitigate the problems were discussed, and implemented.

Results. We show a number of findings by the Gaia FL concerning longer-term evolution, individual but common effects, as well as detrimental impacts, all of which occurred over the operational phase of the Gaia mission

M. Altmann, Z. Balog, W. Löffler, U. Bastian, M. Biermann, A. Sagrista Selles, M. Davidson, N. Rowell, E. Serpell, A. Abreu Aramburu, T. Brüsemeister, C. Crowley, M. Hauser, S. Jordan, J. Martín-Fleitas, A. Mora, E. Fernandez del Peloso, U. Stampa

Comments: 29 pages, 34 figures, accepted for publication in Astronomy & Astrophysics
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2605.03721 [astro-ph.IM](or arXiv:2605.03721v1 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2605.03721
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Related DOI:
https://doi.org/10.1051/0004-6361/202659204
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Submission history
From: Martin Altmann
[v1] Tue, 5 May 2026 13:07:08 UTC (3,890 KB)
https://arxiv.org/abs/2605.03721

Astrobiology, Astronomy, exoplanets, stellar cartography,

Biologist, Explorers Club Fellow, ex-NASA Space Biologist and Payload integrator, Editor of NASAWatch.com and Astrobiology.com, Lapsed climber, Explorer, Synaesthete, Former Challenger Center board member 🖖🏻