Key points are not available for this paper at this time.
The sources of gravitational radiation that seem to be most likely to be detected by planned ground- and space-based gravitational-wave detectors are reviewed, with particular attention to the likely information that observations of them will reveal. A particular emphasis is placed on observations by LISA, the fundamental-physics Cornerstone project of the European Space Agency's Horizon 2000+ programme.
B. F. Schutz (Fri,) studied this question.