  Radiative shocks are strong shocks characterized by plasma at a high
temperature emitting an important fraction of its energy as radiation.
Radiative shocks are commonly found in many astrophysical systems and are
templates of radiative hydrodynamic flows, which can be studied experimentally
using high-power lasers. This is not only important in the context of
laboratory astrophysics but also to benchmark numerical studies. We present
details on the design of experiments on radiative shocks in xenon gas performed
at the kJ scale PALS laser facility. It includes technical specifications for
the tube targets design and numerical studies with the 1-D radiative
hydrodynamics code MULTI. Emphasis is given to the technical feasibility of an
XUV imaging diagnostic with a 21 nm (~58 eV) probing beam, which allows to
probe simultaneously the post-shock and the precursor region ahead of the
shock. The novel design of the target together with the improved X-ray optics
and XUV source allow to show both the dense post-shock structure and the
precursor of the radiative shock.
