  A Euro-Asian network of four gravitational-wave (GW) interferometers is
considered, taking into account the plan to create such a detector in
Novosibirsk. The efficiency of the network is assessed by typical numerical
criteria, which also depend on the characteristics of the received signal. In
this work, we calculate the optimal orientation of the Novosibirsk detector for
the problem of detecting GW radiation accompanying the collapse of the
progenitor star with an initial angular momentum. The specificity of the
scenario is the presence of the so-called. bar stage deformation, for which the
shape of the emitted GW signal is known.
