Fig. 11.
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Differences between the published Gaia colours and XSL colours measured from the spectra. We use response curves for the Gaia photometric system presented by Maíz Apellániz & Weiler (2018, ‘MAW’ in the figure). We exclude stars with temperatures Teff < 4000 K and variable stars from the histogram and rms calculations, but they are still included in the colour-colour comparison for illustrative purposes.
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