  The number of detections as well as significantly deep non-detections of
optical/NIR afterglows of Type I (short-duration population) Gamma-Ray Bursts
(GRBs) has become large enough that statistically meaningful samples can now be
constructed. I present within some recent results on the luminosity
distribution of Type I GRB afterglows in comparison to those of Type II GRBs
(collapsar population), the issue of the existence of jet breaks in Type I GRB
afterglows, and the discovery of dark Type I GRBs.
