Grand Challenges

• A tool allowing a global comparison of a galaxy model (e.g. the one used for the catalogue validation tasks described in WP940) with the actual Gaia data.
• Selection and exploration in the Fourier domain for variability analysis.
• Cross-correlate spatial position and variability information, to explore the structure of our galaxy using variable stars.
• Query per-CCD photometry to explore short-term variability

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