Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 32, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/32/1/015014
Keywords
gravitational waves; black holes; pulsar timing; pulsar timing arrays
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Funding
- Science & Technology Facilities Council
- Science and Technology Facilities Council [1096380] Funding Source: researchfish
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There are several common conventions in use by the gravitational-wave community to describe the amplitude of sources and the sensitivity of detectors. These are frequently confused. We outline the merits of and differences between the various quantities used for parameterizing noise curves and characterizing gravitational-wave amplitudes. We conclude by producing plots that consistently compare different detectors. Similar figures can be generated on-line for general use at http://rhcole.com/apps/GWplotter.
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