Аннотация:The 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.