Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 21, Issue 5, Pages S775-S779Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/21/5/056
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The use of a network of interferometers for the estimation of the position of a transient source of gravitational radiation is discussed in various contexts. The prospects for the observation of electromagnetic counterparts to binary coalescences as well as to more generic gravitational wave bursts are analysed. The requirements for the use of a two-interferometer network to perform a targeted burst search are also discussed.
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