  The existence of FR II objects that are kinetically dominated, the jet
kinetic luminosity, $Q$, is larger than the total thermal luminosity (IR to
X-ray) of the accretion flow, $L_{bol}$, is of profound theoretical interest.
Such objects are not expected in most theoretical models of the central engine
of radio loud AGN. Thus, establishing such a class of objects is an important
diagnostic for filtering through the myriad of theoretical possibilities. This
paper attempts to establish a class of quasars that have existed in a state of
kinetic dominance, $R(t)\equiv Q(t)/L_{bol}(t)>1$, at some epoch, $t$. It is
argued that the 10 quasars in this article with a long term time average
$Q(t)$, $\bar{Q}$, that exceed $L_{Edd}$ are likely to have satisfied the
condition $R(t)>1$ either presently or in the past based on the rarity of
$L_{bol}>L_{Edd}$ quasars. Finally, the existence of these sources is discussed
in the context of the theory of the central engine.
