In later phases of the study, the advice and criticism of the Caltech Gravitational Research Group were sought. Parts of this study have benefited from this interaction, however the tyranny of the schedule to complete this document have left substantial parts of it without their constructive review.
The principal conclusion of this study is that it is timely and feasible to construct a gravitational wave detection system based on at least two long baseline interferometric antennae. The development could open a new field of astrophysics—gravitational astronomy—with its own unique sources and insights into the universe and gravitation. The technical ability exists now to extend the search for gravitational radiation into new frequency bands and to gain a million fold increase in energy sensitivity over present detection systems.
Furthermore, there is substantial margin for further improvement in the sensitivity with technical advances as the fundamental limits for these systems are still many orders of magnitude below the projected sensitivities.
The positive conclusion of this study may have been anticipated. It could have been otherwise: the basic concept could have been flawed, the technology could have been inadequate, and the costs could have been beyond reasons. None of these appears to be the case.
The study is known colloquially as the Blue Book, in reference to the color of its cover.
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