  The newly observed $D_{sJ}^*$ family containing $D_{sJ}^{*}(2317)$,
$D_{sJ}(2460)$ and $D_{sJ}(2632)$ attracts great interests. Determining their
structure may be important tasks for both theorists and experimentalists. In
this work we use the heavy quark effective theory (HQET) and a non-relativistic
model to evaluate the production rate of $D_{sJ}^{*}(2317)$ from the decays of
$\psi(4415)$, and we find that it is sizable and may be observed at BES III and
CLEO, if it is a p-wave excited state of $D_s(1968)$. Unfortunately, the other
two members of the family cannot be observed through decays of charmonia,
because of the constraints from the final state phase space.
