  GRB 020321 is a faint GRB that received wide follow-up attention in X-rays
(BeppoSAX/NFI, Chandra/ACIS-S, XMM-Newton), radio (ATCA) and optical (ESO,
HST). We identify a weak X-ray afterglow by a combined study of the Chandra and
XMM-Newton observations. Its decay index of 1.2 is typical for GRB afterglows.
Inside the 4"-accurate error box there is a weak optical counterpart candidate
with a much shallower decay index.
