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Fig. 3

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Magnitude scatter measured for all the stars located within 20′′ (gray dots) from the RB X-ray position as a function of their magnitude. The black circles highlight all the sources detected within a distance of just 1.5′′ from the RB. The large red star marks the candidate optical counterpart. The top, middle, and bottom panels refer to the F606W, F814W, and Ks filters, respectively.

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