Observed proper eccentricities and proper inclinations of (65) Cybele and other asteroids in its vicinity. We do not find evidence for the existence of a family related to Cybele located at e_p = 0.13 and sin I_p = 0.05 (number ‘65’ along the axis). For comparison, (87) Sylvia and its well-known family are clearly identifiable at e_p = 0.06 and sin I_p = 0.17 (number ‘87’ along the axis). Colours correspond to albedo values from the WISE and AKARI catalogues. Asteroids without albedo measurements are plotted in grey. Symbol sizes are proportional to the logarithm of the diameter.