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Fig. 39

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Distribution of distances for sources detected at 5-σ in the U-band in a Galactic centre field. Distances were obtained by querying the Gaia catalogue for counterparts to the UVOT sources we detect (and retaining only those with at least a 5.0 significance in the parallax, to ensure the distances we retain are reliable). The data is grouped in 40 equally sized bins.

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