Moore, C.J., Cole, R.H. and Berry, C.P.L. (2015) Gravitational-wave sensitivity curves. Classical and Quantum Gravity, 32(1), 015014. (doi: 10.1088/0264-9381/32/1/015014)
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Abstract
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.
| Item Type: | Articles |
|---|---|
| Status: | Published |
| Refereed: | Yes |
| Glasgow Author(s) Enlighten ID: | Berry, Dr Christopher |
| Authors: | Moore, C.J., Cole, R.H., and Berry, C.P.L. |
| College/School: | College of Science and Engineering > School of Physics and Astronomy |
| Journal Name: | Classical and Quantum Gravity |
| Publisher: | IOP Publishing |
| ISSN: | 0264-9381 |
| ISSN (Online): | 1361-6382 |
| Published Online: | 08 December 2014 |
| Copyright Holders: | Copyright © 2015 IOP Publishing Ltd |
| First Published: | First published in Classical and Quantum Gravity 32(1): 015014 |
| Publisher Policy: | Reproduced under a Creative Commons License |
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