Fig. 3
Example of profile analysis for one R image of 523676 (2013 UL10). Left panel: comparison of the four profiles in different directions (grey and blue lines: perpendicular and parallel to the apparent motion of the centaur, respectively; red and green lines: two orthogonal directions oriented at 45° with respectto the two above) around the centaur’s optocentre with the average stellar profile (thick black line). Right panel: comparison of residuals of centaur 523676 (2013 UL10) (filled dots) and 2008 FC76 (empty triangles) with respect to an in-field stellar profile.
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