Absolute magnitude (H) of the asteroids from the Sulamitis and Clarissa families as a function of their proper semi-major axes. Both families are shown in gray. The colored circles correspond to the objects observed in this study. Objects depicted in blue are primitive asteroids (C, X, B, T, and subclasses), while objects in red are non-primitive (A-, V-, and S-types). The family parent asteroids, (752) Sulamitis and (302) Clarissa, are represented as stars and are the largest objects in the families.