A class of radiative solutions of Einstein's field equations with a negativ
e cosmological constant and a pure radiation is investigated. The space-tim
es, which generalize the Defrise solution, represent exact gravitational wa
ves which interact with null matter and propagate in the anti-de Sitter uni
verse. Interestingly, these solutions have homogeneous and non-singular wav
e-fronts for all freely moving observers. We also study properties of sandw
ich and impulsive waves which can be constructed in this class of space-tim
es.