Fig. A.1
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Counts of 67P dust extracted with the aperture sizes corresponding to 1,000 km (black) and 7,500 km (grey) in the cometocentric distance (a) and their differences (b) as a function of wavelength on UT 2016 January 12. We note that α indicates the phase angle on the epoch. In panel (a), black and grey lines overlap and they are indistinguishable from visual inspection.
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