  The Swift/XRT data of 179 GRBs (from 050124 to 070129) and the optical
afterglow data of 57 pre- and post-Swift GRBs are analyzed, in order to
systematically investigate the jet-like breaks in the X-ray and optical
afterglow lightcurves. We find that not a single burst can be included in the
``Platinum'' sample, in which the data satisfy all the criteria of a jet break.
By releasing one or more requirements to define a jet break, some candidates of
various degrees could be identified. In the X-ray band, 42 out of the 103
well-sampled X-ray lightcurves have a decay slope of the post-break segment
>1.5 (``Bronze'' sample), and 27 of them also satisfy the closure relations of
the forward models (``Silver'' sample). The numbers of the ``Bronze'' and
``Silver'' candidates in the optical lightcurves are 27 and 23, respectively.
Thirteen bursts have well-sampled optical and X-ray lightcurves, but only seven
cases are consistent with an achromatic break, but even in these cases only one
band satisfies the closure relations (``Gold'' sample). The observed break time
in the XRT lightcurves is systematically earlier than that in the optical
bands. All these raise great concerns in interpreting the jet-like breaks as
jet breaks and further inferring GRB energetics from these breaks. By assuming
that these breaks are jet breaks, we perform a similar analysis as previous
work to calculate the jet opening angle (theta_j) and energetics (E_k) with the
``Silver'' and ``Gold'' jet break candidates. The derived E_K distribution
reveals a much larger scatter than the pre-Swift sample. A tentative
anti-correlation between theta_j and E_{K,iso} is found for both the pre-Swift
and Swift GRBs, indicating that the E_K could still be quasi-universal, if the
breaks in discussion are indeed jet breaks(abridge).
