Fig. 3
Differential photometry for the second part of night 10, binned per 10 min intervals, obtained with an aperture encompassing both components of the binary (green filled circles), and with apertures encompassing only the PSF centre of Luhman 16A (black empty symbols) and Luhman 16B (red vertical bars). The variations are amplified on Luhman 16B, indicating that they originate from this T-dwarf.
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