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The derivation of information useful for understanding the physics insidecompact stars from HIC observations is a difficult task. Complications due tofinite size, different chemistry, non-adiabatic compression, incompletestopping and structural effects must be overcome. This can only be convincinglyachieved by a successful simulation of many experimental observables varyingincident energy, system size and isospin content. Using now availablesystematic FOPI data in the SIS energy range we try to trace the path to take.

Heavy ion collisions in the 1A GeV regime: how well do we join up to astrophysics?